W. T. Ball, « Solar irradiance variability : a six-year comparison between SORCE observations and the SATIRE model, Astronomy & Astrophysics, vol.530, p.71, 2011.
DOI : 10.1051/0004-6361/201016189
URL : https://www.aanda.org/articles/aa/pdf/2011/06/aa16189-10.pdf

W. T. Ball, « Reconstruction of total solar irradiance 1974, Astronomy & Astrophysics, vol.541, p.27, 2009.

T. Berger, « Magneto-thermal convection in solar prominences, Nature, vol.472, pp.197-200, 2011.

L. Biermann, « Zur Deutung der chromosphärischen Turbulenz und des Exzesses der UV-Strahlung der Sonne, Naturwissenschaften, vol.33, pp.118-119, 1946.

P. Boerner, « Initial Calibration of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO), Solar Physics, vol.275, pp.41-66, 2012.

P. F. Boerner, « Photometric and Thermal Cross-calibration of Solar EUV Instruments, Solar Physics, vol.289, pp.2377-2397, 2014.

J. A. Bonet, I. Cabello, and J. Sánchez-almeida, « Center-to-limb variation of the area covered by magnetic bright points in the quiet Sun, Astronomy & Astrophysics, vol.539, p.6, 2012.

, « Neutrinos from the primary proton-proton fusion process in the Sun, Nature, vol.512, pp.383-386, 2014.

H. Bovensmann, « SCIAMACHY : Mission Objectives and Measurement Modes, Journal of the Atmospheric Sciences, vol.56, issue.2, pp.127-150, 1999.

P. N. Brandt, W. Schmidt, and M. Steinegger, « On the umbrapenumbra area ratio of sunspots, Solar Physics, vol.129, pp.191-194, 1990.

G. E. Brueckner, « The solar ultraviolet spectral irradiance monitor (SUSIM) experiment on board the Upper Atmosphere Research Satellite (UARS), Journal of Geophysical Research, vol.98, p.10, 1993.

P. J. Cargill and J. A. Klimchuk, « Nanoflare Heating of the Corona Revisited, The Astrophysical Journal, vol.605, pp.911-920, 2004.

M. Carlsson, « Can High Frequency Acoustic Waves Heat the Quiet Sun Chromosphere ?, In : Publications of the Astronomical Society of Japan, vol.59, 2007.

C. Cincunegui, R. F. Díaz, and P. J. Mauas, « H? and the Ca II H and K lines as activity proxies for late-type stars, Astronomy & Astrophysics, vol.469, pp.309-317, 2007.

F. Clette, « Revisiting the Sunspot Number. A 400-Year Perspective on the Solar Cycle, Space Science Reviews, vol.186, pp.35-103, 2014.

O. Coddington, « A Solar Irradiance Climate Data Record, Bulletin of the American Meteorological Society, vol.97, p.1265, 2016.

S. Couvidat, « Observables Processing for the Helioseismic and Magnetic Imager Instrument on the Solar Dynamics Observatory, Solar Physics, vol.291, pp.1887-1938, 2016.

A. N. Cox, Allen's astrophysical quantities, 2000.

S. Criscuoli, A. Norton, and T. Whitney, « Photometric Properties of Network and Faculae Derived from HMI Data Compensated for Scattered Light, The Astrophysical Journal, vol.847, p.93, 2017.

T. J. Crowley, « Causes of Climate Change Over the Past 1000, 2000.

. Years, Science 289, pp.270-277

T. Egorova, « Revised historical solar irradiance forcing, Astronomy & Astrophysics, vol.615, p.85, 2018.

I. Ermolli, « Recent variability of the solar spectral irradiance and its impact on climate modelling, Atmospheric Chemistry & Physics, vol.13, pp.3945-3977, 2013.

M. Fligge and S. K. Solanki, « Properties of Flux Tubes and the Relation with Solar Irradiance Variability, Journal of Astrophysics and Astronomy, vol.21, p.275, 2000.

M. Fligge, S. K. Solanki, and Y. C. Unruh, « Modelling irradiance variations from the surface distribution of the solar magnetic field, Astronomy & Astrophysics, vol.353, pp.380-388, 2000.

J. M. Fontenla, E. H. Avrett, and R. Loeser, « Energy balance in the solar transition region. III -Helium emission in hydrostatic, constantabundance models with diffusion, The Astrophysical Journal, vol.406, pp.319-345, 1993.

J. M. Fontenla, « Semiempirical Models of the Solar Atmosphere. III. Set of Non-LTE Models for Far-Ultraviolet/Extreme-Ultraviolet Irradiance Computation, The Astrophysical Journal, vol.707, pp.482-502, 2009.

A. Fossum and M. Carlsson, « Response Functions of the Ultraviolet Filters of TRACE and the Detectability of High-Frequency Acoustic Waves, The Astrophysical Journal, vol.625, pp.556-562, 2005.

P. Foukal, Solar Astrophysics. Physics textbook, 2013.

M. S. Giampapa, L. E. Cram, and W. J. Wild, « The CA II resonance lines in M dwarf stars without H-alpha emission, The Astronomical Journal, vol.345, pp.536-542, 1989.

J. Gomes-da-silva, « On the long-term correlation between the flux in the Ca ii H & K and H? lines for FGK stars, Astronomy & Astrophysics, vol.566, p.66, 2014.

M. Haberreiter, « A new observational solar irradiance composite, Journal of Geophysical Research (Space Physics), vol.122, pp.5910-5930, 2017.

B. N. Handy, « The transition region and coronal explorer, Solar Physics, vol.187, pp.229-260, 1999.

K. L. Harvey and O. R. White, « Magnetic and Radiative Variability of Solar Surface Structures. I. Image Decomposition and Magnetic-Intensity Mapping, The Astrophysical Journal, vol.515, pp.812-831, 1999.

D. H. Hathaway, « Radial Flows in Supergranules, Solar Physics 205, pp.25-38, 2002.

, Solar Prominences. 1 re éd. Astrophysics and Space Science Library 415, pp.978-981, 2015.

F. Kahil, T. L. Riethmüller, and S. K. Solanki, « Brightness of Solar Magnetic Elements As a Function of Magnetic Flux at High Spatial Resolution, The Astrophysical Journal Supplement Series, vol.229, p.12, 2017.

C. Karoff, The Influence of Metallicity on Stellar Differential Rotation and Magnetic Activity, vol.852, p.46, 2018.

P. Kobel, S. K. Solanki, and J. M. Borrero, « The continuum intensity as a function of magnetic field. I. Active region and quiet Sun magnetic elements, Astronomy & Astrophysics, vol.531, p.112, 2011.

G. Kopp, « An assessment of the solar irradiance record for climate studies, Journal of Space Weather and Space Climate 4, vol.27, p.14, 2014.

G. Kopp, K. Heuerman, and G. Lawrence, « The Total Irradiance Monitor (TIM) : Instrument Calibration, Solar Physics, vol.230, pp.111-127, 2005.

G. Kopp, G. Lawrence, and G. Rottman, The Total Irradiance Monitor (TIM) : Science Results, vol.230, pp.129-139, 2005.

A. C. Kren, P. Pilewskie, and O. Et-coddington, , 2017.

, « Where does Earth's atmosphere get its energy ? » In : Journal of Space Weather Space Climate 7, A10

N. A. Krivova, S. K. Solanki, and Y. C. Unruh, « Towards a long-term record of solar total and spectral irradiance, Journal of Atmospheric and Solar-Terrestrial Physics, vol.73, pp.223-234, 2011.

N. A. Krivova, « Reconstruction of solar UV irradiance since, Journal of Geophysical Research (Atmospheres), vol.114, pp.0-04, 1974.

J. R. Kuhn, « The sun's shape and brightness, Nature, vol.392, p.155, 1998.

R. L. Kurucz, « "Finding" the "missing" solar ultraviolet opacity, Revista Mexicana de Astronomia y Astrofisica, vol.23, pp.181-186, 1992.

K. Langhans, « Inclination of magnetic fields and flows in sunspot penumbrae, Astronomy & Astrophysics, vol.436, pp.1087-1101, 2005.

J. R. Lemen, The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO) ». In : Solar Physics, vol.275, pp.17-40, 2012.

Y. Lin, S. F. Martin, and O. Engvold, « Filament Substructures and their Interrelation, Subsurface and Atmospheric Influences on Solar Activity. Sous la dir. de R. Howe et al. T. 383. Astronomical Society of the Pacific Conference Series, p.235, 2008.

Y. Lin, « Thin Threads of Solar Filaments, Solar Physics, vol.226, pp.239-254, 2005.

B. Lites, « Hinode Observations of Horizontal Quiet Sun Magnetic Flux and the "Hidden Turbulent Magnetic Flux" », Publications of the Astronomical Society of Japan, vol.59, pp.571-576, 2007.

B. W. Lites, « Are Internetwork Magnetic Fields in the Solar Photosphere Horizontal or Vertical ?, The Astrophysical Journal, vol.835, p.14, 2017.

W. Livingston, « Sun-as-a-Star Spectrum Variations, The Astrophysical Journal, vol.657, pp.1137-1149, 1974.

S. F. Martin, W. H. Marquette, and R. Bilimoria, « The Solar Cycle Pattern in the Direction of the Magnetic Field along the Long Axes of Polar Filaments, The Solar Cycle. Sous la dir. de K. L. Harvey. T. 27. Astronomical Society of the Pacific Conference Series, p.53, 1992.

S. F. Martin, R. Et-christopher, and . Echols, « An Observational and Conceptual Model of the Magnetic Field of a Filament, pp.339-346, 1994.

K. Matthes, « Solar forcing for CMIP6 (v3.2), Geoscientific Model Development, vol.10, pp.2247-2302, 2017.

M. Mayor, Setting New Standards with HARPS, vol.114, pp.20-24, 2003.

W. E. Mcclintock, G. J. Rottman, and T. N. Woods, « Solar-Stellar Irradiance Comparison Experiment II (Solstice II) : Instrument Concept and Design, Solar Physics, vol.230, pp.225-258, 2005.

N. Meunier, « Solar chromospheric emission and magnetic structures from plages to intranetwork : Contribution of the very quiet Sun, Astronomy & Astrophysics, vol.615, p.87, 2018.

N. Meunier and X. Delfosse, « On the correlation between Ca and H? solar emission and consequences for stellar activity observations, Astronomy & Astrophysics, vol.501, pp.1103-1112, 2009.

, « Filaments and the magnetic configuration. I. Observation of the solar case, Astronomy & Astrophysics, vol.532, p.18, 2011.

N. Meunier, L. Mignon, and A. Lagrange, « Variability in stellar granulation and convective blueshift with spectral type and magnetic activity . II. From young to old main-sequence K-G-F stars, Astronomy & Astrophysics, vol.607, p.124, 2017.

N. Meunier, « Variability of stellar granulation and convective blueshift with spectral type and magnetic activity. I. K and G main sequence stars, Astronomy & Astrophysics, vol.597, 2017.

D. Montes, « Excess H? emission in chromospherically active binaries, Astronomy & Astrophysics, vol.294, pp.165-176, 1995.

G. Narayan and G. B. Scharmer, « Small-scale convection signatures associated with a strong plage solar magnetic field, 524, A3, A3, 2010.

A. A. Norton, « Spectral Line Selection for HMI : A Comparison of Fe I 6173 Å and Ni I 6768 Å, Solar Physics, vol.239, pp.69-91, 2006.

R. W. Noyes, « Rotation, convection, and magnetic activity in lower main-sequence stars, The Astrophysical Journal, vol.279, pp.763-777, 1984.

N. B. Orange, « Temporal Pointing Variations of the Solar Dynamics Observatory's HMI and AIA Instruments on Subweekly Time Scales, Solar Physics, vol.289, pp.1901-1915, 2014.

A. Ortiz, V. Domingo, and B. Sanahuja, « The intensity contrast of solar photospheric faculae and network elements. II. Evolution over the rising phase of solar cycle 23, Astronomy & Astrophysics, vol.452, pp.311-319, 2006.

A. Ortiz, « On the intensity contrast of solar photospheric faculae and network elements, Astronomy & Astrophysics, vol.388, pp.1036-1047, 2002.

M. J. Owens, « The Maunder minimum and the Little Ice Age : an update from recent reconstructions and climate simulations, Journal of Space Weather and Space Climate, vol.7, p.33, 2017.

S. Parenti, « Solar Prominences : Observations, Living Reviews in Solar Physics, vol.11, issue.1, pp.1614-4961, 2014.

E. N. Parker, « Topological Dissipation and the Small-Scale Fields in Turbulent Gases, The Astrophysical Journal, vol.174, p.499, 1972.

L. Pasquini and R. Pallavicini, « H-alpha absolute chromospheric fluxes in G and K dwarfs and subgiants, Astronomy & Astrophysics, vol.251, pp.199-209, 1991.

M. J. Penn and W. Livingston, Temporal Changes in Sunspot Umbral Magnetic Fields and Temperatures, vol.649, pp.45-48, 2006.

M. J. Penn and R. K. Macdonald, « Solar Cycle Changes in Sunspot Umbral Intensity, The Astrophysical Journal, vol.662, pp.123-126, 2007.

W. D. Pesnell, B. J. Thompson, and P. C. Chamberlin, « The Solar Dynamics Observatory (SDO), Solar Physics, vol.275, pp.3-15, 2012.

K. J. Phillips, Ultraviolet and x-ray spectroscopy of the solar atmosphere, vol.44, 2008.

E. Priest, Magnetohydrodynamics of the Sun, 2014.

M. P. Rast, « Sunspot Bright Rings : Evidence from Case Studies, The Astrophysical Journal, vol.557, pp.864-879, 2001.

R. D. Robinson, L. E. Cram, and M. S. Giampapa, « Chromospheric H-alpha and CA II lines in late-type stars, The Astrophysical Journal, Supplement, vol.74, pp.891-909, 1990.

G. Rottman, « The SORCE Mission, Solar Physics, vol.230, pp.7-25, 2005.

T. Roudier, « Relation between trees of fragmenting granules and supergranulation evolution, Astronomy & Astrophysics, vol.590, p.121, 2016.

S. Sanchez, A. Fournier, and J. Aubert, « The Predictability of Advection-dominated Flux-transport Solar Dynamo Models, The Astrophysical Journal, vol.781, p.8, 2014.

P. H. Scherrer, « The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO) ». In : Solar Physics 275, pp.207-227, 2012.

J. Schou, « Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO), Solar Physics, vol.275, pp.229-259, 2012.

C. J. Schrijver, « Simulations of the Photospheric Magnetic Activity and Outer Atmospheric Radiative Losses of Cool Stars Based on Characteristics of the Solar Magnetic Field, The Astrophysical Journal, vol.547, pp.475-490, 2001.

M. Schwarzschild, « On Noise Arising from the Solar Granulation, The Astrophysical Journal, vol.107, p.1, 1948.

S. Sofia and L. H. Li, « Solar variability and climate, Journal of Geophysics Research, vol.106, pp.12969-12974, 2001.

S. K. Solanki, « Sunspots : An overview, The Astronomy & Astrophysics Review, vol.11, pp.153-286, 2003.

S. K. Solanki, N. A. Krivova, and J. D. Haigh, « Solar Irradiance Variability and Climate, Annual Review of Astronomy & Astrophysics, vol.51, pp.311-351, 2013.

H. Spruit, « Theory of solar irradiance variations, Space Science Reviews, vol.94, pp.113-126, 2000.

H. C. Spruit, « Effect of spots on a star's radius and luminosity, Astronomy & Astrophysics, vol.108, pp.348-355, 1982.

, « The flow of heat near a starspot, Astronomy & Astrophysics, vol.108, pp.356-360, 1982.

K. G. Strassmeier, « Chromospheric CA II H and K and Halpha emission in single and binary stars of spectral types F6-M2, The Astrophysical Journal, Supplement, vol.72, pp.191-230, 1990.

J. H. Thomas, O. Et-nigel, and . Weiss, Sunspots and Starspots. Cambridge Astrophysics, 2008.

Y. C. Unruh, S. K. Solanki, and M. Fligge, « The spectral dependence of facular contrast and solar irradiance variations, Astronomy & Astrophysics, vol.345, pp.635-642, 1999.

I. G. Usoskin, « A History of Solar Activity over Millennia, Living Reviews in Solar Physics, vol.10, p.1, 2013.

J. E. Vernazza, E. H. Avrett, and R. Loeser, « Structure of the solar chromosphere. III -Models of the EUV brightness components of the quietsun, The Astrophysical Journal Supplement Series, vol.45, pp.635-725, 1981.

M. Waldmeier, Astronomische Mitteilungen der Eidgenössischen Sternwarte Zurich, vol.14, pp.439-450, 1939.

G. L. Withbroe, « Quiet Sun Contribution to Variations in the Total Solar Irradiance, Solar Physics, vol.235, pp.369-386, 2006.

. Bibliographie,

C. L. Wolff and J. R. Hickey, « Solar irradiance change and special longitudes due to r-modes, Science, vol.235, pp.1631-1633, 1987.

T. Woods, « Solar Irradiance Variability : Comparisons of Observations over Solar Cycles 21-24, EGU General Assembly Conference Abstracts. Sous la dir. d'A. Abbasi et N. Giesen. T. 14. EGU General Assembly Conference Abstracts, p.1520, 2012.

T. N. Woods, G. Rottman, and R. Vest, « XUV Photometer System (XPS) : Overview and Calibrations, Solar Physics, vol.230, pp.345-374, 2005.

K. L. Yeo, « Point spread function of SDO/HMI and the effects of stray light correction on the apparent properties of solar surface phenomena, Astronomy & Astrophysics, vol.561, p.22, 2014.

K. L. Yeo, S. K. Solanki, and N. A. Krivova, « Intensity contrast of solar network and faculae, Astronomy & Astrophysics, vol.550, p.95, 2013.

K. L. Yeo, « Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI, and SDO/HMI observations, Astronomy & Astrophysics, vol.570, p.85, 2014.