Physikalisch-Meteorologisches Observatorium Davos Space experiments of PMOD/WRC to measure the solar constant and the influence of the solar irradiance on the terrestrial climate Werner Schmutz PMOD/WRC ISPMSRS'07 12-14 March 2007 Davos, Switzerland PMOD 1907-2007 WRC since 1971 Two activities: Operational Service Guided tour at PMOD/WRC for ISPMSRS'07 participants „World Radiation Center“ Energy balance and influence of radiation on the terrestrial climate ¾ Green house effect ¾ Sun-Earth connection 12.3.2007 = calibration of meteorological instruments Monday measuring 2 pm radiation Tuesday 2 pm Research Overview 1 Physikalisch-Meteorologisches Observatorium Davos Overview • Past observations of the Total Solar Irradiance (TSI) and the TSI-composite • Why irradiance measurements • Why continue to measure TSI 12.3.2007 • Future irradiance observations Absolutely calibrated TSI observations TIM/SORCE 12.3.2007 2003 - Overview 2 Physikalisch-Meteorologisches Observatorium Davos A side note: Need for improved Quality Assurance! Difficulties: - Bias between sensors MISR, MODIS, AVHRR ….. On-board calibration systems expensive! Reliable? Traceable? BIPM and WMO are proposing Inter-team / manufacturer /agency on launch andpreparing degrade and adebate meeting in 2008 in-orbit Need for agreement orspectral) 2009 dedicated to International calibration (gain and No consistent statements of and traceability problems uncertainty or “degrees of - Instruments change 12.3.2007 confidence”. Courtesy of Nigel Fox Traceable Radiometry Underpinning Terrestrial- & Helio- Studies Mission proposal: TRUTHS Nigel Fox NPL Nigel.Fox@npl.co.uk U of Alab. Mike Sandford RAL Plym Mar Lab Michael Schaepman U of Zur Xavier Briottet ONERA Werner Schmutz PMOD/WRC John Barnett Ox univ. Keith Shine Uni of Read Steve Groom Plym Mar Lab Phil Teillet CCRS Claus Frohlich PMOD/WRC Theo Theocharous NPL Jo Haigh Imp Coll Kurtis Thome U of Ariz Olivier Hagolle CNES Terry Quinn BIPM Hugh Kieffer USGS Michel Verstraete JRC(Italy) Judith Lean NRL Emma Woolliams NPL John Martin NPL Ed Zalewski U of Ariz 12.3.2007 James Aiken David Pollock Overview 3 Physikalisch-Meteorologisches Observatorium Davos TSI – including TIM/SORCE Absolute measurements cannot be used to construct a long-term record 12.3.2007 Æ Merge to a relative composite TSI – comparisons of different composites 12.3.2007 Different composites predict different long-term trends: Overview Courtesy of Claus Fröhlich 4 Physikalisch-Meteorologisches Observatorium Davos Why irradiance measurements? IUGG 2007: On short term, the T., solar influence on the terrestrial Rozanov E., Egorova Schmutz W., Peter T., 2006: • Space Weather: atmosphere dominated by the variations Session MS020 Simulation ofisthe stratospheric ozone and of the Monitoring of220 thenm solar Totalband) and Spectral UV (Ly-α and Herzberg temperature to the solar Solar Activityresponse and its Influences onirradiance the Earth's irradiance variability during sun rotation Weather Climate (IRC) Influenceand of the short-term (dayscycle to months) variations on JASTP 68, 2203composition of the upper terrestrial atmosphere the chemical 12.3.2007 • Space Climate: Long term record the Solar On long term, it is notofknown what Irradiance dominates, Influence of the long-term variations on the chemical secular change of Total Solar Irradiance or composition of the upper terrestrial atmosphere and its spectral (UV) variations propagation to the troposphere changing the terrestrial climate But: although UV variations are much larger (up to 100%) all spectral variations are highly correlated to TSI variations What is the influence of the Sun on the climate? 12.3.2007 ? Overview Graphics: Dr. J. Beer EAWAG, Switzerland 5 Physikalisch-Meteorologisches Observatorium Davos Climate Anomalies versus solar influence River Thames in London 1813/1814 200 Maunder Dalton 150 100 12.3.2007 50 0 1600 1650 1700 1750 1800 YEAR 1850 1900 1950 2000 illustration: Dr. J. Beer EAWAG, Switzerland Predicted long-term trend of TSI 100 years 12.3.2007 Different “educated” guesses! Overview 6 Physikalisch-Meteorologisches Observatorium Davos Predicted long-term trend of TSI 400 years Suspected secular change of TSI needs to be confirmed observationally Different “educated” Æ requires long term observation of several decades! 12.3.2007 guesses! Three minima in the latest (August 2006) version of the PMOD-composite The present minimum is It is essential 0.15 to design W/m (= 110the ppm) lower than the previous irradiance measurements at the twoagree minimain their value to The three minima highest possible accuracy! or 60 ppm) within ±0.08 W/m2 (0.006% 2 12.3.2007 Î Solution: twin instrument experiment as VIRGO on SoHO and PREMOS+SOVAP on PICARD Overview The latest (updated) composite is published on the PMOD/WRC web site http:www.pmodwrc.ch follow the links: Æ projects Æ Solar Constant / Solar Irradiance 7 Physikalisch-Meteorologisches Observatorium Davos VIRGO/SoHO: operational since 1996 12.3.2007 • Two absolute radiometers: - PMO6V (A & B) - DIARAD (L & R) • Precision Filter Radiometer (blue, green, red) • Image of the Sun in the green light in low resolution (12 pixels): 1 minute sampling SoHO launch 2. December 1995 DIARAD PMO6 SPM LOI VIRGO instruments Future TSI experiments ¾ GLORY (USA: no launch date – ready to be used as gap-filler) ¾ SOVIM/ISS and ¾ PREMOS+SOVAP/PICARD approved TSI experiments of PMOD/WRC 12.3.2007 ¾ RAD/KuaFu-A only future TSI experiment presently being considered Overview 8 Physikalisch-Meteorologisches Observatorium Davos 12.3.2007 Space experiments are being built in house at PMOD/WRC Space experiments of PMOD/WRC 12.3.2007 today Overview 9 Physikalisch-Meteorologisches Observatorium Davos PICARD (PI G. Thuillier) PREMOS – SOVAP – SODISM 12.3.2007 Filter Radiometers Total Solar Irradiance Total Solar Irradiance observations until 2012 ACRIM III 2000 - ? VIRGO/SOHO 1996 TIM/SORCE 2003 - 2009 (+?) 2008 - (?) 12.3.2007 SOVIM/ISS 2008 – 2009 ? PREMOS/PICARD 2009 – 2011 SOVAP/PICARD (SDO 2008-2012 has no TSI instrument) Overview NPOESS 2012 TSI o National Polar Orbiting n NPO Operational Environmental Satellite E Sc ancele – but are planned to start System may have TSI Sinstrument d June not earlier than 2009 (?), more likely as20late 06 as 2012 10 Physikalisch-Meteorologisches Observatorium Davos Total Solar Irradiance observations until 2012 ACRIM III 2000 - ? VIRGO/SOHO 1996 2007 2009 TIM/SORCE 2003 – 2008 - (GLORY?) SOVIM/ISS PREMOS-TSI/PICARD SOVAP/PICARD 2007 - 2009 ? 2009 - 2013 (SDO 2008-2012 has no TSI instrument) KuaFu-A irradiance measurement experiment comprising: 2012 - 12.3.2007 Æ SIM = Solar Irradiance Monitor (CN: PI Daren Lu) Æ DOR = Davos Observatory Radiometer (CH: Werner Schmutz) Conclusions Short-term irradiance variations (days) are closely related to variations of the chemical composition of the upper atmosphere Æ space weather: operational monitoring of TSI • Long-term irradiance variations (tens to thousands of years) are probably (!) related to climate variations Æ space climate: secular long term change of TSI • TSI observations are most likely continuous and overlapping until about 2012 • RAD/KuaFu-A would be a matching continuation 12.3.2007 • Overview 11 Physikalisch-Meteorologisches Observatorium Davos Thank you for your attention! Integration of LYRA on PROBA2 5.3.2007 Overview 12