| Issue |
J. Space Weather Space Clim.
Volume 4, 2014
Solar variability, solar forcing, and coupling mechanisms in the terrestrial atmosphere
|
|
|---|---|---|
| Article Number | A30 | |
| Number of page(s) | 11 | |
| DOI | https://doi.org/10.1051/swsc/2014027 | |
| Published online | 17 October 2014 | |
- Barra, V., V. Delouille, and J.-F. Hochedez, Segmentation of extreme ultraviolet solar images via multichannel fuzzy clustering, Adv. Space Res., 42, 917–925, DOI: 10.1016/j.asr.2007.10.021, 2008. [Google Scholar]
- BenMoussa, A., S. Gissot, U. Schühle, G. Del Zanna, F. Auchère, et al., On-orbit degradation of solar instruments, Sol. Phys., 288, 389–434, DOI: 10.1007/s11207-013-0290-z, 2013. [Google Scholar]
- Bezdek, J., Pattern recognition with fuzzy objective function algorithms, Plenum Press, New-York, 1981. [Google Scholar]
- Bochsler, P., H. Kucharek, E. Möbius, M. Bzowski, J.M. Sokół, L. Didkovsky, and S. Wieman, Solar photoionization rates for interstellar neutrals in the inner heliosphere: H, He, O, and Ne, Astrophys. J. Suppl. Ser., 210, 12, DOI: 10.1088/0067-0049/210/1/12, 2014. [Google Scholar]
- Cessateur, G., T. Dudok de Wit, M. Kretzschmar, J. Lilensten, J.-F. Hochedez, and M. Snow, Monitoring the solar UV irradiance spectrum from the observation of a few passbands, A&A, 528, A68, DOI: 10.1051/0004-6361/201015903, 2011. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Cessateur, G., J. Lilensten, T. Dudok de Wit, A. BenMoussa, and M. Kretzschmar, New observation strategies for the solar UV spectral irradiance, J. Space Weather Space Clim., 2, A16, DOI: 10.1051/swsc/2012016, 2012. [CrossRef] [EDP Sciences] [Google Scholar]
- Clette, F., J.-F. Hochedez, J.S. Newmark, J.D. Moses, F. Auchère, J.-M. Defise, and J.-P. Delaboudinière, The radiometric calibration of the extreme ultraviolet imaging telescope, ISSI Scientific Reports Series, 2, 121, 2002. [Google Scholar]
- Delaboudinière, J.-P., G.E. Artzner, J. Brunaud, A.H. Gabriel, J.F. Hochedez, et al., EIT: Extreme-ultraviolet Imaging Telescope for the SOHO mission, Sol. Phys., 162, 291–312, DOI: 10.1007/BF00733432, 1995. [NASA ADS] [CrossRef] [Google Scholar]
- Dere, K.P., E. Landi, H.E. Mason, B.C. Monsignori Fossi, and P.R. Young, CHIANTI – an atomic database for emission lines, Astron. Astrophys. Suppl. Ser., 125, 149–173, DOI: 10.1051/aas:1997368, 1997. [CrossRef] [EDP Sciences] [Google Scholar]
- Didkovsky, L.V., D.L. Judge, A.R. Jones, S. Wieman, and B.T. Tsurutani, Correction of SOHO CELIAS/SEM EUV measurements saturated by extreme solar flare events, Astron. Nachr., 328, 36–40, DOI: 10.1002/asna.200610667, 2007. [NASA ADS] [CrossRef] [Google Scholar]
- Didkovsky, L.V., D.L. Judge, S.R. Wieman, and D. McMullin. Minima of solar cycles 22/23 and 23/24 as seen in SOHO/CELIAS/SEM absolute solar EUV flux. In: S.R., Cranmer, J.T. Hoeksema, and J.L. Kohl, Editors,Astronomical Society of the Pacific Conference Series, 428, 73, 2010. [Google Scholar]
- Dominique, M., J.-F. Hochedez, W. Schmutz, I.E. Dammasch, A.I. Shapiro, M. Kretzschmar, A.N. Zhukov, D. Gillotay, Y. Stockman, and A. BenMoussa, The LYRA instrument onboard PROBA2: description and in-flight performance, Sol. Phys., 286, 21–42, DOI: 10.1007/s11207-013-0252-5, 2013. [NASA ADS] [CrossRef] [Google Scholar]
- Dudok de Wit, T., and S. Bruinsma, Determination of the most pertinent EUV proxy for use in thermosphere modeling, Geophys. Res. Lett., 38, L19102, DOI: 10.1029/2011GL049028, 2011. [CrossRef] [Google Scholar]
- Dudok de Wit, T., S. Bruinsma, and K. Shibasaki, Synoptic radio observations as proxies for upper atmosphere modelling, J. Space Weather Space Clim., 4, A06, DOI: 10.1051/swsc/2014003, 2014. [CrossRef] [EDP Sciences] [Google Scholar]
- Fontenla, J.M., W. Curdt, M. Haberreiter, J. Harder, and H. Tian, Semiempirical models of the solar atmosphereIII. Set of non-LTE models for far-ultraviolet/extreme-ultraviolet irradiance computation, Astrophys. J., 707, 482–502, DOI: 10.1088/0004-637X/707/1/482, 2009. [Google Scholar]
- Fontenla, J.M., J. Harder, W. Livingston, M. Snow, and T. Woods, High-resolution solar spectral irradiance from extreme ultraviolet to far infrared, J. Geophys. Res. (Atmos.), 116, D20108, DOI: 10.1029/2011JD016032, 2011. [CrossRef] [Google Scholar]
- Haberreiter, M., Solar EUV spectrum calculated for quiet sun conditions, Sol. Phys., 274, 473–479, DOI: 10.1007/s11207-011-9767-9, 2011. [NASA ADS] [CrossRef] [Google Scholar]
- Haberreiter, M.. Towards the reconstruction of the EUV irradiance for solar cycle 23. In: C.H., Mandrini, and D.F. Webb, Editors, IAU Symposium, 286, 97–100, DOI: 10.1017/S174392131200470X, 2012. [Google Scholar]
- Haberreiter, M., W. Schmutz, and A.G. Kosovichev, Solving the discrepancy between the seismic and photospheric solar radius, Astrophys. J., 675, L53–L56, DOI: 10.1086/529492, 2008. [CrossRef] [Google Scholar]
- Hinteregger, H.E., K. Fukui, and B.R. Gilson, Observational reference and model data on solar EUV, from measurements on AE-E, Geophys. Res. Lett., 8, 1147–1150, 1981. [Google Scholar]
- Hochedez, J., W. Schmutz, Y. Stockman, U. Schühle, A. Benmoussa, et al., LYRA, a solar UV radiometer on Proba2, Adv. Space Res., 37, 303–312, DOI: 10.1016/j.asr.2005.10.041, 2006. [NASA ADS] [CrossRef] [Google Scholar]
- Hovestadt, D., M. Hilchenbach, A. Bürgi, B. Klecker, P. Laeverenz, et al., CELIAS – Charge, Element and Isotope Analysis System for SOHO, Sol. Phys., 162, 441–481, DOI: 10.1007/BF00733436, 1995. [NASA ADS] [CrossRef] [Google Scholar]
- Judge, D.L., D.R. McMullin, H.S. Ogawa, D. Hovestadt, B. Klecker, et al., First solar EUV irradiances obtained from SOHO by the CELIAS/SEM, Sol. Phys., 177, 161–173, DOI: 10.1023/A:1004929011427, 1998. [NASA ADS] [CrossRef] [Google Scholar]
- Kretzschmar, M., I.E. Dammasch, M. Dominique, J. Zender, G. Cessateur, and E. D’Huys, Extreme ultraviolet solar irradiance during the rising phase of solar cycle 24 observed by PROBA2/LYRA, J. Space Weather Space Clim., 2, A14, DOI: 10.1051/swsc/2012014, 2012. [CrossRef] [EDP Sciences] [Google Scholar]
- Kretzschmar, M., J. Lilensten, and J. Aboudarham, Retrieving the solar EUV spectral irradiance from the observation of 6 lines, Advances in Space Research, 37, 341–346, DOI: 10.1016/j.asr.2005.02.029, 2006. [Google Scholar]
- Krishnapuram, R., and J. Keller, A possibilistic approach to clustering, IEEE Trans. Fuzzy Systems, 1, 98–110, 1993. [Google Scholar]
- Krishnapuram, R., and J. Keller, The possibilistic C-means algorithm: Insights and recommendations, IEEE Trans. Fuzzy Systems, 4, 385–393, 1996. [CrossRef] [Google Scholar]
- Landi, E., G. Delzanna, P.R. Young, K.P. Dere, H.E. Mason, and M. Landini, CHIANTI-An atomic database for emission lines. VII. New data for X-rays and other improvements, Astrophys. J. Suppl. Ser., 162, 261–280, DOI: 10.1086/498148, 2006. [Google Scholar]
- Laštovička, J., Are trends in total electron content (TEC) really positive, J. Geophys. Res. (Space Phys.), 118, 3831–3835, DOI: 10.1002/jgra.50261, 2013 [CrossRef] [Google Scholar]
- Lean, J.L., J.T. Emmert, J.M. Picone, and R.R. Meier, Global and regional trends in ionospheric total electron content, J. Geophys. Res. (Space Phys.), 116, A00H04, DOI: 10.1029/2010JA016378, 2011a. [Google Scholar]
- Lean, J.L., T.N. Woods, F.G. Eparvier, R.R. Meier, D.J. Strickland, J.T. Correira, and J.S. Evans, Solar extreme ultraviolet irradiance: Present, past, and future, J. Geophys. Res. (Space Phys.), 116, A01102, DOI: 10.1029/2010JA015901, 2011b. [Google Scholar]
- Lemen, J.R., A.M. Title, D.J. Akin, P.F. Boerner, C. Chou, et al., The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO), Sol. Phys., 275, 17–40, DOI: 10.1007/s11207-011-9776-8, 2012. [NASA ADS] [CrossRef] [Google Scholar]
- Lilensten, J., T. Dudok de Wit, M. Kretzschmar, P.-O. Amblard, S. Moussaoui, J. Aboudarham, and F. Auchère, Review on the solar spectral variability in the EUV for space weather purposes, Ann. Geophys., 26, 269–279, 2008. [NASA ADS] [CrossRef] [Google Scholar]
- McMullin, D.R., D.L. Judge, M. Hilchenbach, F. Ipavich, P. Bochsler, P. Wurz, A. Burgi, W.T. Thompson, and J.S. Newmark, In-flight comparisons of solar EUV irradiance measurements provided by the CELIAS/SEM on SOHO, ISSI Scientific Reports Series, 2, 135, 2002. [Google Scholar]
- Ogawa, H.S., D.R. McMullin, D.L. Judge, and R.S. Korde, Normal incidence spectrophotometer with high-density transmission grating technology and high-efficiency silicon photodiodes for absolute solar extreme-ultraviolet irradiance measurement, Opt. Eng., 32, 3121–3125, DOI: 10.1117/12.149195, 1993. [CrossRef] [Google Scholar]
- Qian, L., and S.C. Solomon, Thermospheric density: an overview of temporal and spatial variations, Space Sci. Res., 168, 147–173, DOI: 10.1007/s11214-011-9810-z, 2012. [Google Scholar]
- Schmidtke, G., R. Brunner, D. Eberhard, B. Halford, U. Klocke, M. Knothe, W. Konz, W.-J. Riedel, and H. Wolf, SOL-ACES: Auto-calibrating EUV/UV spectrometers for measurements onboard the International Space Station, Adv. Space Res., 37, 273–282, DOI: 10.1016/j.asr.2005.01.112, 2006a. [NASA ADS] [CrossRef] [Google Scholar]
- Schmidtke, G., C. Fröhlich, and G. Thuillier, ISS-SOLAR: Total (TSI) and spectral (SSI) irradiance measurements, Adv. Space Res., 37, 255–264, DOI: 10.1016/j.asr.2005.01.009, 2006b. [NASA ADS] [CrossRef] [Google Scholar]
- Thuillier, G., J. Claudel, D. Djafer, M. Haberreiter, N. Mein, S.M.L. Melo, W. Schmutz, A. Shapiro, C.I. Short, and S. Sofia, The shape of the solar limb: Models and observations, Sol. Phys., 268, 125–149, DOI: 10.1007/s11207-010-9664-7, 2011. [NASA ADS] [CrossRef] [Google Scholar]
- Thuillier, G., G. Schmidtke, C. Erhardt, B. Nikutowski, A.I. Shapiro, et al., Solar spectral irradiance variability in November/December 2012: Comparison of observations by instruments on the international space station and models, Sol. Phys., DOI: 10.1007/s11207-014-0588-5, 2014. [Google Scholar]
- Verbeeck, C., V. Delouille, B. Mampaey, and R. De Visscher, The SPoCA-suite: Software for extraction, characterization, and tracking of active regions and coronal holes on EUV images, A&A, 561, A29, DOI: 10.1051/0004-6361/201321243, 2014. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Warren, H.P., J.T. Mariska, and J. Lean, A new model of solar EUV irradiance variability: 1. Model formulation, J. Geophys. Res., 106, 15,745–15,758, DOI: 10.1029/2000JA000282, 2001. [Google Scholar]
- Wieman, S.R., L.V. Didkovsky, and D.L. Judge, Resolving differences in absolute irradiance measurements between the SOHO/CELIAS/SEM and the SDO/EVE, Sol. Phys., 289, 2907–2925, DOI: 10.1007/s11207-014-0519-5, 2014. [NASA ADS] [CrossRef] [Google Scholar]
- Wieman, S.R., D.L. Judge, and L.V. Didkovsky, Solar EUV Monitor (SEM) absolute irradiance measurements and how they are affected by choice of reference spectrum. Proc. SPIE, 8148, DOI: 10.1117/12.893163, 2011. [Google Scholar]
- Woods, T.N., F.G. Eparvier, S.M. Bailey, P.C. Chamberlin, J. Lean, G.J. Rottman, S.C. Solomon, W.K. Tobiska, and D.L. Woodraska, Solar EUV Experiment (SEE): mission overview and first results, J. Geophys. Res. (Space Phys.), 110, A01312, DOI: 10.1029/2004JA010765, 2005. [CrossRef] [Google Scholar]
- Woods, T.N., F.G. Eparvier, R. Hock, A.R. Jones, D. Woodraska, et al., Extreme ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of science objectives, instrument design, data products, and model developments, Sol. Phys., 275, 115–143, DOI: 10.1007/s11207-009-9487-6, 2012. [Google Scholar]
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