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Sunlight-JAD 2014

Authors:
  • Mental Health Institute Hospital del Mar
Research report
Relationship between sunlight and the age of onset of bipolar disorder:
An international multisite study
Michael Bauer
a,
n
, Tasha Glenn
b
, Martin Alda
c
, Ole A. Andreassen
d
, Elias Angelopoulos
e
,
Raffaella Ardau
f
, Christopher Baethge
g
, Rita Bauer
a
, Frank Bellivier
h,i
,
Robert H. Belmaker
j
, Michael Berk
k,l,m
, Thomas D. Bjella
d
, Letizia Bossini
n
,
Yuly Bersudsky
j
, Eric Yat Wo Cheung
o
,Jörn Conell
a
, Maria Del Zompo
p
, Seetal Dodd
k,q
,
Bruno Etain
r,i
, Andrea Fagiolini
n
, Mark A. Frye
s
, Kostas N. Fountoulakis
t
,
Jade Garneau-Fournier
u
, Ana González-Pinto
v
, Hirohiko Harima
w
, Stefanie Hassel
x
,
Chantal Henry
r,i
, Apostolos Iacovides
t
, Erkki T. Isometsä
y,z
, Flávio Kapczinski
aa
,
Sebastian Kliwicki
ab
, Barbara König
ac
, Rikke Krogh
ad
, Mauricio Kunz
aa
, Beny Lafer
ae
,
Erik R. Larsen
ad
, Ute Lewitzka
a
, Carlos Lopez-Jaramillo
af
, Glenda MacQueen
x
,
Mirko Manchia
c
, Wendy Marsh
ag
, Mónica Martinez-Cengotitabengoa
v
, Ingrid Melle
d
,
Scott Monteith
ah
, Gunnar Morken
ai
, Rodrigo Munoz
aj
, Fabiano G. Nery
ae
,
Claire ODonovan
c
, Yamima Osher
j
, Andrea Pfennig
a
, Danilo Quiroz
ak
, Raj Ramesar
al
,
Natalie Rasgon
u
, Andreas Reif
am
, Philipp Ritter
a
, Janusz K. Rybakowski
ab
,
Kemal Sagduyu
an
, Ângela M. Scippa
ao
, Emanuel Severus
a
, Christian Simhandl
ac
,
Dan J. Stein
ap
, Sergio Strejilevich
aq
, Ahmad Hatim Sulaiman
ar
, Kirsi Suominen
as
,
Hiromi Tagata
w
, Yoshitaka Tatebayashi
at
, Carla Torrent
au
, Eduard Vieta
au
,
Biju Viswanath
av
, Mihir J. Wanchoo
s
, Mark Zetin
aw
, Peter C. Whybrow
ax
a
Department of Psychiatry and Psychotherapy, University Hospital Carl Gustav Carus, Technische Universität, Dresden, Germany
b
ChronoRecord Association, Fullerton, CA, USA
c
Department of Psychiatry, Dalhousie University, Halifax, NS, Canada
d
NORMENT K.G. Jebsen Centre for Psychosis Research, Division of Mental Health and Addiction, Oslo University Hospital &Institute of Clinical Medicine,
Oslo, Norway
e
Department of Psychiatry, University of Athens Medical School, Eginition Hospital, Athens, Greece
f
Unit of Clinical Pharmacology, University-Hospital of Cagliari, Sardinia, Italy
g
Department of Psychiatry and Psychotherapy, University of Cologne Medical School, Cologne, Germany
h
Psychiatrie, GH Saint-Louis Lariboisière F. Widal, APHP, INSERM UMR-S1144, Faculté de Médecine, Université D. Diderot, Paris, France
i
FondaMental Fondation, Créteil, France
j
Department of Psychiatry, Faculty of Health Sciences, Ben Gurion University of the Negev, Beer Sheva Mental Health Center, Beer Sheva, Israel
k
IMPACT Strategic Research Centre, School of Medicine, Deakin University, Geelong, Victoria 3220, Australia
l
Department of Psychiatry, ORYGEN Youth Health Research Centre, Centre for Youth Mental Health, Australia
m
The Florey Institute for Neuroscience and Mental Health, University of Melbourne, Parkville, Victoria 3052, Australia
n
Department of Molecular Medicine and Department of Mental Health (DAI), University of Siena and University of Siena Medical Center (AOUS), Siena, Italy
o
Department of General Adult Psychiatry, Castle Peak Hospital, Hong Kong
p
Section of Neurosciences and Clinical Pharmacology, Department of Biomedical Sciences, University of Cagliari, Sardinia, Italy
q
Department of Psychiatry, University of Melbourne, Parkville, Victoria 3052, Australia
r
AP-HP, Hopitaux Universitaires Henri Mondor and INSERM U955 (IMRB), Université Paris Est, Creteil, France
s
Department of Psychiatry &Psychology, Mayo Clinic Depression Center, Mayo Clinic, Rochester, MN, USA
t
3rd Department of Psychiatry, Division of Neurosciences, School of Medicine, Aristotle University of Thessaloniki, Thessaloniki, Greece
u
Department of Psychiatry and Behavioral Sciences, Stanford School of Medicine, Palo Alto, CA, USA
v
Department of Psychiatry, University Hospital of Alava, University of the Basque Country, CIBERSAM, Vitoria, Spain
w
Department of Psychiatry, Tokyo Metropolitan Matsuzawa Hospital, Setagaya, Tokyo, Japan
x
Department of Psychiatry, Faculty of Medicine, University of Calgary, Calgary, AB, Canada
y
Department of Psychiatry, Institute of Clinical Medicine, University of Helsinki, Finland
z
National Institute for Health and Welfare, Helsinki, Finland
aa
Laboratory of Molecular Psychiatry, Hospital de Clínicas de Porto Alegre, Federal University of Rio Grande do Sul, Porto Alegre, Brazil
ab
Department of Adult Psychiatry, Poznan University of Medical Sciences, Poznan, Poland
ac
BIPOLAR Zentrum Wiener Neustadt, Wiener Neustadt, Austria
ad
Department of Affective Disorders, Q, Mood Disorders Research Unit, Aarhus University Hospital, Denmark
ae
Bipolar Disorder Research Program, Department of Psychiatry, University of São Paulo Medical School, São Paulo, Brazil
Contents lists available at ScienceDirect
journal homepage: www.elsevier.com/locate/jad
Journal of Affective Disorders
http://dx.doi.org/10.1016/j.jad.2014.05.032
0165-0327/&2014 Elsevier B.V. All rights reserved.
Journal of Affective Disorders 167 (2014) 104111
af
Mood Disorders Program, Fundacion San Vicente de Paul, Department of Psychiatry, Universidad de Antioquia, Medellín, Colombia
ag
Department of Psychiatry, University of Massachusetts, Worcester, MA, USA
ah
Michigan State University College of Human Medicine, Traverse City Campus, Traverse City, MI, USA
ai
Department of Neuroscience, NTNU, and St OlavsUniversity Hospital, Trondheim, Norway
aj
Department of Psychiatry, University of California San Diego, San Diego, CA, USA
ak
Deparment of Psychiatry, Diego Portales University, Santiago, Chile
al
UCT/MRC Human Genetics Research Unit, Institute of Infectious Disease and Molecular Medicine, University of Cape Town, Cape Town, South Africa
am
Department of Psychiatry, Psychosomatics and Psychotherapy, University of Würzburg, Würzburg, Germany
an
Department of Psychiatry, University of Missouri Kansas City, School of Medicine, Kansas City, MO, USA
ao
Department of Neuroscience and Mental Health, Federal University of Bahia, Salvador, Brazil
ap
Department of Psychiatry, University of Cape Town, Cape Town, South Africa
aq
Bipolar Disorder Program, Neuroscience Institute, Favaloro University, Buenos Aires, Argentina
ar
Department of Psychological Medicine, Faculty of Medicine, University of Malaya, Kuala Lumpur, Malaysia
as
City of Helsinki, Department of Social Services and Health Care, Psychiatry, Helsinki, Finland
at
Schizophrenia &Affective Disorders Research Project, Tokyo Metropolitan Institute of Medical Science, Seatagaya, Tokyo, Japan
au
Clinical Institute of Neuroscience, Hospital Clinic, University of Barcelona, IDIBAPS, CIBERSAM, Barcelona, Catalonia, Spain
av
Department of Psychiatry, NIMHANS, Bangalore 560029, India
aw
Department of Psychology, Chapman University, Orange, CA, USA
ax
Department of Psychiatry and Biobehavioral Sciences, Semel Institute for Neuroscience and Human Behavior, University of California Los Angeles (UCLA),
Los Angeles, CA, USA
article info
Article history:
Received 28 February 2014
Received in revised form
20 May 2014
Accepted 21 May 2014
Available online 29 May 2014
Keywords:
Bipolar disorder
Age of onset
Sunlight
Insolation
abstract
Background: The onset of bipolar disorder is inuenced by the interaction of genetic and environmental
factors. We previously found that a large increase in sunlight in springtime was associated with a lower
age of onset. This study extends this analysis with more collection sites at diverse locations, and includes
family history and polarity of rst episode.
Methods: Data from 4037 patients with bipolar I disorder were collected at 36 collection sites in 23
countries at latitudes spanning 3.2 north (N) to 63.4 N and 38.2 south (S) of the equator. The age of onset
of the rst episode, onset location, family history of mood disorders, and polarity of rst episode were
obtained retrospectively, from patient records and/or direct interview. Solar insolation data were
obtained for the onset locations.
Results: There was a large, signicant inverse relationship between maximum monthly increase in solar
insolation and age of onset, controlling for the country median age and the birth cohort. The effect was
reduced by half if there was no family history. The maximum monthly increase in solar insolation
occurred in springtime. The effect was one-third smaller for initial episodes of mania than depression.
The largest maximum monthly increase in solar insolation occurred in northern latitudes such as Oslo,
Norway, and warm and dry areas such as Los Angeles, California.
Limitations: Recall bias for onset and family history data.
Conclusions: A large springtime increase in sunlight may have an important inuence on the onset of
bipolar disorder, especially in those with a family history of mood disorders.
&2014 Elsevier B.V. All rights reserved.
1. Introduction
Sunlight provides warmth, stimulates vision, initiates vitamin
D synthesis, and plays a fundamental role in how the circadian
clock adapts human physiology and behavior to the alternation of
day and night (Berson, 2003; Brainard and Hanin, 2005; Hatori
and Panda, 2010). Circadian rhythms are involved in regulation
of mood (Albrecht, 2010; McClung, 2013) and abnormalities
in circadian rhythms are thought to underlie bipolar disorder
(Goodwin and Jamison, 1990; Mansour et al., 2005; McClung,
2007). We previously found that the larger the springtime increase
in solar electromagnetic energy striking the surface of the earth
(insolation) at the onset location, the younger the age of onset of
bipolar disorder (Bauer et al., 2012).
The emergence of bipolar disorder involves the interaction of
complex genetic mechanisms (Burmeister et al., 2008; Craddock
and Sklar, 2013; Petronis, 2003) and environmental factors
(Tsuchiya et al., 2003). Based on 6 studies of 2509 patients with
bipolar I disorder, the weighted mean age of onset falls into
3 groups, having peaks at ages 18.1, 26.9 and 42.7 years, with
55% of patients in the middle or late onset groups (Bellivier et al.,
2001, 2003; González Pinto et al., 2009; Hamshere et al., 2009; Lin
et al., 2006; Manchia et al., 2008). This broad range of onset and
the polygenic basis of bipolar disorder suggest that environmental
factors have an inuential role (Burmeister et al., 2008; Craddock
and Sklar, 2013; Wright et al., 2003). Environmental factors
associated with a younger age of onset are cannabis use
(González-Pinto et al., 2008; Lagerberg et al., 2011), stressful life
events (Horesh et al., 2011) and childhood abuse (Garno et al.,
2005; Leverich et al., 2002), while neurological illness is associated
with an older onset (Depp and Jeste, 2004). The purpose of this
study was to repeat our prior investigation of the association
between solar insolation and the age of onset of bipolar disorder
using a substantially larger sample, and including information on
family history and polarity of the rst episode.
2. Methods
2.1. Patient data
All patients included in this study had a diagnosis of bipolar
disorder according to DSM-IV criteria made by a psychiatrist.
Approval for this study was obtained from institutional review
boards according to local requirements. Patient data were
n
Corresponding author. Tel.: þ49 351 458 0; fax: þ49 30 450 51 79 62.
E-mail address: michael.bauer@uniklinikum-dresden.de (M. Bauer).
M. Bauer et al. / Journal of Affective Disorders 167 (2014) 104111 105
obtained retrospectively at 36 collection sites in 23 countries.
In 20 sites (Athens, Greece; Bangalore, India; Buenos Aires,
Argentina; Cagliari, Sardinia, Italy; Dresden, Germany; Halifax,
Canada; Helsinki, Finland; Hong Kong; Kansas City, KS, USA;
Los Angeles, CA, USA; Medellín, Colombia; Oslo, Norway; Paris,
France; Porto Alegre, Brazil; Rochester, MN, USA; San Diego, CA,
USA; Santiago, Chile; Siena, Italy; Thessaloniki, Greece; Würzburg,
Germany), data were gathered by direct interviews and reviewing
records, in 8 sites (Barcelona, Spain; Melbourne/Geelong,
Australia; Palo Alto, CA, USA; São Paulo, Brazil; Salvador, Brazil;
Trondheim, Norway; Vitoria-Basque Country, Spain; Worcester,
MA, USA) primarily by direct interviews, and at the remaining
8 sites (Aarhus, Denmark; Beer Sheva, Israel; Calgary, Canada;
Cape Town, South Africa; Kuala Lumpur, Malaysia; Poznan, Poland;
Tokyo, Japan; Wiener Neustadt, Austria) primarily by reviewing
records.
Variables included sex, date of birth, age of onset, location of
onset, family history of any mood disorder in a rst degree
relative, and polarity of the rst episode (depressed, manic or
hypomanic). The age of onset was dened as the rst occurrence
of an episode of depression, mania or hypomania according to
DSM-IV criteria.
2.2. Potential confounders
Apart from any solar insolation effects, there were two potential
age-related confounders. The country median age varied by about 20
years between the oldest (Japan 45.8 years) and youngest (South
Africa at 25.5) collection sites. For a disease with a variable age of
onset that spans several decades, an older age of onset would be
expected in a country with an older population (Chen et al., 1993;
Heimbuch et al., 1980). The country median age was included in all
models to reect the differences in country population.
Previous research reported a large birth cohort effect in bipolar
disorder with an older onset in older cohorts (Chengappa et al.,
2003), and that less than 10% of people develop bipolar disorder after
age 50 (Vasudev and Thomas, 2010). Since the current data includes a
largepercentageofpeoplebornbefore1960(36.8%),threebirth
cohort groups were created: born before 1940, born between 1940
and 1959, and born after 1959 (Chengappa et al., 2003). The birth
cohort grouping variable was included in all models.
There was a large imbalance in the percent of patients with a
diagnosis of bipolar I disorder as compared to other bipolar
subtypes. Since the percent of bipolar I varied from 23% to 99%,
with 40% of collection sites having Z80% of patients with bipolar I
disorder, only patients with a diagnosis of bipolar I disorder were
included in the analysis.
2.3. Solar insolation data
All solar insolation data were obtained from the USA National
Aeronautics and Space Administration (NASA) Surface Meteorol-
ogy and Solar Energy (SSE) Version 6.0 database, which is based on
data collected over a 22 year time period from 1983 to 2005
(NASA, 2012). Average monthly solar insolation data are available
for the entire globe with a spatial resolution of 1 11latitude/
longitude. Solar insolation is a measure of the electromagnetic
energy from the sun received for a given surface area on earth at
a given time, expressed in kWh/m
2
/day (kilowatt hours/square
meter/day). Solar insolation is not evenly distributed across the
earth's surface. The solar insolation varies with the annual changes
to the earthsun relationship (angle of incidence which the sun's
rays strike the earth, the day length, and the latitude), reection,
scattering and absorption of the sun's rays by clouds and aerosols
in the atmosphere, and reection back into space by snow, ice, and
desert sand on the earth's surface (NASA, 2010).
The overall pattern of monthly changes to solar insolation
varies greatly by latitude. At the equator, there is very little change
to solar insolation throughout the year. Generally, the closer to the
poles, the greater the range in solar insolation across the year. See
Fig. 1 for examples of monthly changes in insolation at collection
sites in this study. Additionally, locations at the same latitude may
have very different solar insolation due to local conditions such as
cloud cover, altitude, and proximity to large bodies of water. For
example, Rome, Italy and Chicago IL, USA have the same latitude of
41.91north (N) and the same hours of daylight. However the
maximum monthly increase in solar insolation is 1.4 kWh/m
2
/day
in Rome but only 1.01 kWh/m
2
/day in Chicago, occurring between
February and March for both cities.
2.4. Solar insolation variables
Onset location data from every patient were grouped into
reference cities. Each reference city represents all locations within
the 1 11grid of latitude and longitude. For example, Dresden
with latitude of 51.1 N and 13.81east (E) is the reference city for
all onset locations between 51 and 521N, and 13 and 141E. The
monthly solar insolation data for reference cities in the southern
hemisphere were shifted by 6 months to be comparable with
monthly solar insolation in the northern hemisphere. The number
of reference cities from each collection site varied considerably
reecting country size, migration patterns and cultural differences.
Monthly, yearly and seasonal variables were created using the
solar insolation data for each reference city including the monthly
increase and decrease in solar insolation, the yearly cumulative solar
insolation, and the yearly minimum and maximum monthly solar
insolation. The interaction between maximum monthly increase in
solar insolation family history, and maximum monthly increase in
solar insolation polarity of rst episode were also analyzed.
2.5. Country specic variables
The variables available for each country for each reference city
included the lifetime prevalence of bipolar I disorder, the country
median age, and the country sex ratio for ages 1564 (CIA World
Factbook).
Fig. 1. Comparison of monthly solar insolation pattern at northern, equatorial and
temperate latitudes. The pattern of monthly solar insolation at Helsinki, Finland
(60.2 N), San Francisco, CA, USA (37.8 N) and Medellín, Columbia (6.3 N).
M. Bauer et al. / Journal of Affective Disorders 167 (2014) 104111106
2.6. Statistics
Generalized Estimating Equations (GEE) models were used to
estimate the effect of solar insolation on the age of onset. The GEE
method corrects for the correlated data within each reference city
(cluster) (Zeger and Liang, 1986), estimates the difference in
magnitude of the association between two variables through the
use of interaction terms, and estimates the effect across the entire
population rather than within a cluster. All GEE models used age of
onset as the dependent variable. An exchangeable correlation
matrix was chosen, as appropriate for a large number of clusters
with variable cluster sizes including many with a single observa-
tion (Stedman et al., 2008; Zeger and Liang, 1986). To further
evaluate the birth cohort effect, models were also estimated that
excluded both patients born before 1960 and the birth cohort
variable. The model t was assessed using the quasi-likelihood
independent model criterion that is suitable for GEE (Pan, 2001).
A signicance level of 0.01 was used to evaluate estimated
coefcients. Sidak's adjustment was used to evaluate multiple
comparisons at the 0.01 level. SPSS Version 22 was used for all
analyses.
3. Results
Data were collected for a total of 5465 patients. Of the 5465
patients, 4037 had a diagnosis of bipolar I disorder, 1236 had
bipolar II and 192 had bipolar NOS. Only the 4037 patients with
a diagnosis of bipolar I disorder were included in the analysis. The
4037 patients included 2414 from the prior analysis (Bauer et al.,
2012). Of the 4037 patients, 2374 (58.8%) were female and 1663
(41.2%) were male. Family history was available for 3334 (82.6%) of
the 4037 patients and polarity of rst episode was available for
3600 (89.2%).
The mean age of the patients was 48.1714.5 years. For
comparison with prior international studies, the unadjusted age
of onset for the 4037 patients was 25.4710.7 years, similar to
previous reports of 25.7 years, n¼1665 (Baldessarini et al., 2012)
and 25.6 years, n¼1041 ( Morselli et al., 2003). Of the 4037
patients, 220 (5.4%) were born before 1940, 1267 (31.4%) were
born between 1940 and 1959, and 2550 (63.2%) were born after
1959. As expected, country median age and birth cohort were
signicantly associated with the age of onset (both po0.001).
Although data for the 4037 patients were collected at 36
collection sites in 23 countries, the onset locations were in 318
unique reference cities or clusters in 43 countries. The onset loca-
tion was in northern hemisphere for 2994 patients and in the
southern hemisphere for 1043 patients. The distribution of the
onset locations across latitudes is shown in Table 1. The mean
number of patients in each reference city was 12.7 with 4.3% of the
4037 patients in a reference city of one.
The best tting model included the interaction of the max-
imum monthly increase in solar insolation family history, the
country median age and the birth cohort. This is labeled Model 1.
The primary result was an inverse relationship between maximum
monthly increase in solar insolation and age of onset, which was
reduced by about 50% if there was no family history. To put these
results in perspective, when comparing 2 regions with a difference
of 0.1 kWh/m
2
/day in the maximum monthly increase in solar
insolation, the region with the larger increase is associated with a
0.49 year or nearly 6 months younger age of onset when there is a
family history of bipolar disorder, as compared to the region with
the smaller increase. If there is no family history, this difference is
reduced to 0.26 year or about 3 months. There were similar results
when Model 1 was run excluding patients born before 1960 and
the birth cohort. Model 2 included the interaction of the max-
imum monthly increase in solar insolation polarity of rst
episode, the country median age and the birth cohort, and was
also signicant. The results also showed the inverse relationship
between maximum monthly increase in solar insolation and age
of onset, but the effect was about 1/3 smaller for initial episodes
of mania. Similar results for Model 2 were also obtained
when excluding patients born before 1960 and the birth cohort.
See Tables 2 and 3.
The maximum monthly increase in solar insolation occurred in
springtime: between February and March in 40% of onset loca-
tions, between March and April in 38% of onset locations, and
between April and May in 11% of onset locations, excluding the
locations near the equator that have little monthly change in solar
insolation throughout the year. The maximum increase in solar
insolation occurred in diverse latitudes. Table 4 shows the mean
age of onset adjusted for country median age and birth cohort by
the maximum monthly increase in solar insolation.
The collection site was thought to adequately serve as a proxy
for the specic onset location for patients from Barcelona, Cape
Town, Helsinki, Melbourne/Geelong, Porto Alegro, São Paulo,
Salvador, Vitoria, and Würzburg. The best tting model was run
excluding all these sites and the magnitude of the estimated
coefcients did not change substantially and remained signicant
at the 0.01 level.
The age of onset was also associated with the range of monthly
solar insolation but the model was not as good a t as with the
maximum monthly increase. As in our prior study, the yearly
cumulative solar insolation, the maximum decrease in monthly
solar insolation, the yearly minimum and maximum monthly solar
insolation, latitude, sex, country prevalence of bipolar I disorder,
and country sex ratio were not signicantly associated with the
age of onset.
4. Discussion
The maximum monthly increase in solar insolation in spring-
time was inversely associated with the age of onset of bipolar
disorder, but this effect was reduced by half in those without
a family history of mood disorders. This nding replicated the
results of our initial study (Bauer et al., 2012) with a sample that is
67% larger in size and contains 77% more reference cities. The
interaction with family history suggests there may be a genetic
predisposition to some physiological responses to sunlight, and
highlights the importance of obtaining a family history from all
patients. This nding is also consistent with many prior reports
that family history is associated with a younger age of onset
(Baldessarini et al., 2012; Lin et al., 2006; Post et al., 2013;
Schürhoff et al., 2000).
Both the collection sites and the onset locations were distrib-
uted across all latitudes in both hemispheres, and represent a wide
Table 1
Patient onset location by latitude.
Degrees latitude (north and south)
a
Number of patients
09 309
1019 200
2029 286
3039 1222
4049 1475
5059 297
6069 247
7079 1
Total 4037
a
1043 in southern hemisphere.
M. Bauer et al. / Journal of Affective Disorders 167 (2014) 104111 107
range of solar insolation proles including arid, sub-arctic, equa-
torial as well as temperate. In locations that experience a large
increase in sunlight in springtime, detailed questioning to detect
symptoms of bipolar disorder, and closer monitoring of patients
and their adolescent children may be indicated. Conversely, in
locations with little change in sunlight throughout the year, the
onset of bipolar disorder may be at an older age than expected
from studies conducted in temperate climates. The effect of the
maximum monthly increase in solar insolation on the age of onset
is one-third smaller for those with a rst episode of mania rather
than depression, in line with prior observation that a rst episode
of depression occurs at a younger age than mania (Forty et al.,
2009; Ortiz et al., 2011; Perlis et al., 2005).
Both longstanding clinical observation of circadian dysfunction
in bipolar disorder, and active ongoing research into circadian
genes and phenotypes support the concept that a large monthly
increase in solar insolation may be associated with disease onset
(Goodwin and Jamison, 1990; Mansour et al., 2005; McCarthy
et al., 2012; McClung, 2007; Whybrow, 1997). The recent progress
in understanding how light changes are unconsciously captured
and transmitted to the circadian system (Benarroch, 2011; Foster
and Hankins, 2007; Hatori and Panda, 2010) may someday help to
explain the solar insolation ndings in this study. Photosensitive
retinal ganglion cells (pRGC) containing the pigment melanopsin
mediate a broad range of non-image forming functions including
circadian synchronization, melatonin suppression and alertness
(Berson, 2003, Gooley et al., 2003; Zaidi et al., 2007). The intrinsic
photosensitivity of pRGC is specialized to detect uctuations in
intensity of environmental light (Berson, 2003, Hatori and Panda,
2010) and the signals are sent to the circadian pacemaker in the
suprachiasmatic nucleus (SCN). The peak spectral absorption for
non-image forming functions is at short wavelength of visible
light, or blue light: 480 nm for of melanopsin (Berson et al.,
2002), 460 nm for melatonin suppression (Brainard et al., 2001),
and 470 nm for alertness (Stephenson et al., 2012). Similarly, the
dominant wavelength of morning sunlight was measured at
477 nm in the USA (Gallagher III et al., 1996; Turner and
Mainster, 2008).
Although people who live at latitudes with a short daylength have
less exposure to solar insolation during winter, indoor lighting is
optimized for vision (Andersen et al., 2012; van Bommel, 2006; van
Bommel and van den Beld, 2004). In contrast to circadian photo-
reception, peak absorptions for vision are at longer wavelength:
rod-mediated dim light vision at 506 nm or green light, and cone-
mediated bright/moderate light vision at 555 nm or green-yellow
light (Turner and Mainster, 2008). Standard lighting, such as incan-
descent, uorescent warm, and low pressure sodium lamps, has
a dominant wavelength of about 575 nm (Bellia et al., 2011)andless
than 5% of the intensity of sunlight. However, unlike with vision,
insufcient circadian light exposure is not perceived (Turner et al.,
2010). There are ongoing efforts to develop new standards for indoor
lighting that address circadian as well as visual effects, and will
consider the spectrum, intensity, timing of exposure, duration of
signal, and ocular physiology (Andersen et al., 2012; Bellia et al.,
2011; van Bommel and van den Beld, 2004).
While blue light may be the most important component
of solar insolation from a circadian perspective, its role in the
emergence of bipolar disorder is not known. The spectral compo-
sition of sunlight varies with the time of day, season and latitude
(Thorne et al., 2009) and younger people may be particularly
Table 2
Estimated parameter coefcients explaining age of onset with all patients
a
.
Parameter Coefcient
estimate
Standard
error
99% Condence interval Coefcient signicance
Lower Upper Wald chi-square P
Model 1 N¼3334
b
Maximum monthly increase in solar insolation 4.862 1.496 8.678 0.973 10.412 0.001
No family history maximum monthly increase in solar insolation 2.310 0.311 1.510 3.110 55.271 o0.001
Model 2 N¼3600
c
Maximum monthly increase in solar insolation 4.948 1.732 9.409 0.487 8.161 0.004
First episode manic maximum monthly increase in solar insolation 1.663 0.400 0.633 2.694 17.301 o0.001
a
GEE model estimated age of onset using a constant, the country of onset median age, birth cohort groups and the listed parameters with an exchangeable correlation
structure in each cluster. The Wald hypothesis test degrees of freedom were 1 for all models.
b
256 Onset locations. All Sidak pairwise mean age of onset comparisons for birth cohort and family history were signicantly different at the o0.001 level.
c
265 Onset locations. All Sidak pairwise mean age of onset comparisons for birth cohort and rst episode were signicantly different at the o0.001 level.
Table 3
Estimated parameter coefcients explaining age of onset with patients born after 1959
a
.
Parameter Coefcient
estimate
Standard
error
99% Condence interval Coefcient signicance
Lower Upper Wald Chi-square P
Model 1 N¼2091
b
Maximum monthly increase in solar insolation 4.623 1.407 8.247 0.998 10.792 0.001
No family history maximum monthly increase in solar insolation 1.809 0.265 1.127 2.492 46.622 o0.001
Model 2 N¼2271
c
Maximum monthly increase in solar insolation 4.880 1.429 8.561 1.199 11.661 0.001
First episode manic maximum monthly increase in solar insolation 2.213 0.337 1.345 3.081 43.129 o0.001
a
GEE model estimated age of onset using a constant, the country of onset median age and the listed parameters with an exchangeable correlation structure in each
cluster. The Wald hypothesis test degrees of freedom were 1 for all models.
b
216 Onset locations.
c
223 Onset locations.
M. Bauer et al. / Journal of Affective Disorders 167 (2014) 104111108
sensitive to a springtime increase in blue light. Young eyes only
need about half the circadian illuminance as middle aged eyes due
to age-related decreases in pupil area and crystalline lens trans-
mission (Turner et al., 2010). In animal studies, abnormal light
cycles increased depression-like behavior and impaired learning in
normal mice, but not in mice without pRGC (LeGates et al., 2012).
Blue light exposure also stimulates cognitive brain activity in
normal and blind individuals as detected by fMRI (Stephenson
et al., 2012; Vandewalle et al., 2007; Vandewalle et al., 2013).
Preliminary studies of patients with seasonal affective disorder
(SAD) found blue light treatment to be more effective than red
light (Anderson et al., 2009; Glickman et al., 2006 ), and that
sequence variation in the melanopsin gene may increase vulner-
ability to SAD (Roecklein et al., 2009).
Other recent evidence supports the importance of a large monthly
increase in solar insolation. In patients with depression, there were
more early responders to paroxetine when sunlight was increasing
during springtime (Tomita et al., 2012). Seasonal variation with an
increase in the springsummer months was reported in the serum
concentration of brain-derived neurotropic factor (BDNF) (Molendijk
et al., 2012) and in serotonin turnover in cerebrospinal uid (Luykx
et al., 2013), and these may be involved in the pathophysiology of
depression. Dose dependent suppression of melatonin by light (West
et al., 2011) may be exaggerated in bipolar I disorder (Hallam et al.,
2009). Vitamin D synthesis in skin requires sunlight exposure. Low
vitamin D concentrations were associated with diverse psychiatric
disorders (Berk et al., 2008), and by meta-analysis, with depression
(Anglin et al., 2013; Annweiler et al., 2013) and poor cognition (Balion
et al., 2012). Finally, some patients with depression show anomalies in
the retinal response to light (Fountoulakis, 2010; Fountoulakis et al.,
2005).
4.1. Limitations
There are several limitations to this study. The diagnosis
of bipolar disorder was based on the DSM-IV criteria, but the
processes of diagnostic assessment and data gathering were not
standardized across the collection sites. Self-reported age of onset
data are subject to recall bias, however this approach was used in
related research (Baldessarini et al., 2012; Forty et al., 2009; Lin
et al., 2006; Perlis et al., 2005). Family history data is often
inaccurate and more reliable for severe disorders (Hardt and
Franke, 2007), and may be inuenced by cultural attitudes towards
mental illness (Karasz, 2005). Individual exposure to sunlight such
as for outdoor workers was not assessed, although most people in
industrialized countries work indoors and have indoor hobbies
(Godar, 2005; Pergams and Zaradic, 2008). This study did not
include other environmental factors that may affect the age of
onset such as drug abuse, or factors known to disrupt circadian
rhythms such as night shift work or irregular lifestyles (Kapczinski
Table 4
Mean adjusted age of onset by maximum monthly increase in solar insolation (kWh/m
2
/day) groups.
Maximum monthly
increase in solar
insolation (kWh/m
2
/day)
Mean adjusted
age of onset
Number of onset
reference sites
Number of
patients
Percent of
patients
Example locations Latitude (deg)
o0.75 27.53 22 779 19 Kuala Lumpur, Malaysia 3.17 N
Medellín, Columbia 6.29 N
Bangalore, India 12.98 N
Salvador, Brazil 12.98 S
Hong Kong, China 22.25 N
Tokyo, Japan 35.69 N
Z0.75 and o1.0 22.47 47 133 3 Kedah, Malaysia 6.13 N
Kolar, India 13.13 N
Miami, FL, USA 25.78 N
Princeton, NJ, USA 40.35 N
Boston, MA, USA 42.35 N
Z1.0 and o1.25 20.97 136 1756 44 Porto Alegre, Brazil 30.03 S
San Diego, CA, USA 32.71 N
Buenos Aires, Argentina 34.60 S
Melbourne, Australia 37.81 S
Thessaloniki, Greece 40.64 N
Barcelona, Spain 41.38 N
Siena, Italy 43.32 N
Rochester, MN, USA 44.02 N
Nova Scotia, Canada 45.10 N
Vienna, Austria 48.20 N
Paris, France 48.87 N
Würzburg, Germany 49.79 N
Z1.25 and o1.5 20.82 85 707 18 Beer Sheva, Israel 31.25 N
Valparaiso, Chile 33.05 S
San Francisco, CA, USA 37.78 N
Sardinia, Italy 39.22 N
Bordeaux, France 44.83 N
Calgary, Canada 51.08 N
Poznan, Poland 51.42 N
Z1.5 19.32 28 662 16 Santiago, Chile 33.45 S
Cape Town, South Africa 33.92 S
Los Angeles, CA, USA 34.05 N
Aarhus, Denmark 56.16 N
Helsinki, Finland 60.18 N
Trondheim, Norway 63.42 N
Total 318 4037 100
M. Bauer et al. / Journal of Affective Disorders 167 (2014) 104111 109
et al., 2011; Rosa et al., 2013). Shifting data from the southern
hemisphere by six months ignores local cultural dimensions of
seasonality.
4.2. Conclusions
In conclusion, the monthly increase in solar insolation may
have a signicant impact on the age of onset of bipolar disorder,
especially in those with a family history of mood disorders.
The larger the maximum monthly increase in solar insolation
in springtime, the younger the onset of bipolar disorder. A rst
episode of depression occurred at a younger age than mania,
despite the effects of a large springtime increase in solar insola-
tion. Research into the effects of the duration, intensity, timing and
wavelength of light is needed in bipolar disorder.
Role of funding source
This work was funded in part by the Canadian Institutes of Health Research
(MA, Grant number 64410); the Research Council of Norway (OAA Grant numbers
213837; 223273; 217776); South-East Norway Health Authority (OAA, Grant
number 2013-123); a NHMRC Senior Principal Research Fellowship (M Berk, Grant
number 1059660; INSERM (BE, Grant number C0829) and APHP (BE, Grant number
AOR11096); the Spanish Government (AGP, Grant numbers PS09/02002 CIBER
Network; EC10-333, PI10/01430, PI10/01746, PI11/01977, PI11/02708, 2011/1064,
11-BI-01, 1677-DJ-030, EC10-220); European Regional Development Funds (Grant
numbers UE/2012/FI-STAR, UE/2013/TENDERMH, UE/2013/MASTERMIND), grants
from Spanish Government (Grant numbers PI10/01430, PI10/01746, EC10-220,
EC10-333, PI11/01977, 20111064, PI11/02708, PI12/02077, PI13/02252, PI13/
00451), local grants from the Basque Government (Grant numbers 200911147,
20 1011117 0, 201011 20 09 , 2011111110, 20 11111113) ; th e Basque Foundation for
Health Innovation and Research (Grant number BIO12/AL/002); the Spanish Clinical
Research Network (Grant numbers CAIBER;1392-D-079) and the University of the
Basque Country (Grant number IT679-13); Stanley Research Foundation (Grant
number 03-RC-003); the Research Council of Norway (IM, Grant numbers
ES488722, ES421716); the Regional Health Authority of South Eastern Norway
(IM, Grants number 2011085, 2013088); DFG (AR, Grant numbers SFB TRR 58, B06,
Z02); the DFG and Länder funds (AR, Grant number RTG1252/2); Medical Research
Council of South Africa (DJS); Spanish Ministry of Economy and Competitiveness
(EV, Grants number PI12/00912, PN 2008-2011); the Instituto de Salud Carlos III-
Subdirección General de Evaluación y Fomento de la Investigación (EV); Fondo
Europeo de Desarrollo Regional Unión Europea. Una manera de hacer Europa (EV);
CIBERSAM (EV); the Comissionat per a Universitats i Recerca del DIUE de la
Generalitat de Catalunya to the Bipolar Disorders Group (EV, Grant number 2009
SGR 1022). MB, EA, RA, CB, FB, RB, RHB, TDB, LB, YB, EYWC, MDZ, SD, AF, MAF, KNF,
JGF, TG, HH, SH, CH, AI, ETI, FK, SK, BK, RK, MK, BL, ERL, CLJ, UL, GM, MM, WM, SM,
RM, FGN, CO, YO, AP, DQ, RR, NR, PR, JKR, KS, AMS, ES, CS, SS, AHS, KS, HT, YT, CT, BV,
MJW, MZ and PCW have no specic funding to acknowledge. The funding sources
had no involvement in the study design, collection, analysis and interpretation of
data, in writing the report, and in the decision to submit for publication.
Conict of interest
The authors have no conict of interest to declare.
Acknowledgments
We would like to thank the International Society of Bipolar Disorders for
supporting this project.
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