|
Thermal Non-equilibrium Revealed by Periodic Pulses of Random Amplitudes in Solar Coronal Loops,
Auchère, F., Froment C., Bocchialini K., Buchlin E., and Solomon J.
, The Astrophysical Journal, Volume 827, (2016)
|
|
Solar irradiance observations with PREMOS filter radiometers on the PICARD mission: In-flight performance and data release,
Cessateur, G., Schmutz W., Wehrli C., Gröbner J., Haberreiter M., Kretzschmar M., Rozanov E., Schöll M., Shapiro A., Thuillier G., et al.
, Astronomy & Astrophysics, Volume 588, p.A126, (2016)
|
|
Hydrogen Ly-α and Ly-β full Sun line profiles observed with SUMER/SOHO (1996-2009),
Lemaire, P., Vial J.-C., Curdt W., Schühle U., and Wilhelm K.
, Astronomy & Astrophysics, Volume 581, p.A26, (2015)
|
|
Evidence for Evaporation-incomplete Condensation Cycles in Warm Solar Coronal Loops,
Froment, C., Auchère F., Bocchialini K., Buchlin E., Guennou C., and Solomon J.
, The Astrophysical Journal, Volume 807, Issue 2, p.158, (2015)
|
|
The Balmer Lines of He ii in the Blue Wing of the Hydrogen Lyman α Line Observed in a Quiescent Prominence,
Vial, J.-C., Eurin G., and Curdt W.
, Solar Physics, Volume 290, Issue 2, p.381-387, (2015)
|
|
Non-LTE modelling of prominence fine structures using hydrogen Lyman-line profiles,
Schwartz, P., Gunár S., and Curdt W.
, Astronomy & Astrophysics, Volume 577, p.A92, (2015)
|
|
Joining the yellow hub: Uses of the Simple Application Messaging Protocol in Space Physics analysis tools,
Genot, V., Andre N., Cecconi B., Bouchemit M., Budnik E., Bourrel N., Gangloff M., Dufourg N., Hess S., Modolo R., et al.
, Astronomy and Computing, Volume 7, p.62-70, (2014)
|
|
The SUMER Data in the SOHO Archive,
Curdt, W., Germerott D., Wilhelm K., Schühle U., Teriaca L., Innes D., Bocchialini K., and Lemaire P.
, Solar Physics, Volume 289, Issue 6, p.2345-2376, (2014)
|
|
On the formation of Mg ii h and k lines in solar prominences,
Heinzel, P., Vial J.-C., and Anzer U.
, Astronomy & Astrophysics, Volume 564, p.A132, (2014)
|
|
Long-period intensity pulsations in the solar corona during activity cycle 23,
Auchère, F., Bocchialini K., Solomon J., and Tison E.
, Astronomy & Astrophysics, Volume 563, p.A8, (2014)
|
|
Time Evolution of the Altitude of an Observed Coronal Wave,
Delannée, C., Artzner G., Schmieder B., and Parenti S.
, Solar Physics, Volume 289, Issue 7, p.2565-2585, (2014)
|
|
Solar Prominences: Observations,
Parenti, S.
, Living Reviews in Solar Physics, Volume 11, Issue 1, (2014)
|
|
TomograPy: A Fast, Instrument-Independent, Solar Tomography Software,
Barbey, N., Guennou C., and Auchère F.
, Solar Physics, Volume 283, p.227-245, (2013)
|
|
Coronal Temperature Maps from Solar EUV Images: A Blind Source Separation Approach,
Dudok_de_Wit, T., Moussaoui S., Guennou C., Auchère F., Cessateur G., Kretzschmar M., Vieira L. A., and Goryaev F. F.
, Solar Physics, Mar, Volume 283, p.31-47, (2013)
|
|
Can the Differential Emission Measure Constrain the Timescale of Energy Deposition in the Corona?,
Guennou, C., Auchère F., Klimchuk J. A., Bocchialini K., and Parenti S.
, The Astrophysical Journal, Volume 774, Issue 1, p.31, (2013)
|
|
Nature and Variability of Plasmas Ejected by the Sun,
Vial, J.-C.
, The Environments of the Sun and the Stars, Volume 857, Number ISBN 978-3-642-30647-1, p.15, (2013)
|
|
Flows at the Edge of an Active Region: Observation and Interpretation,
Boutry, C., Buchlin E., Vial J.-C., and Régnier S.
, Astrophysical Journal, Volume 752, p.13, (2012)
|
|
The solar hydrogen Lyman α to Lyman β line ratio,
Lemaire, P., Vial J.-C., Curdt W., Schühle U., and Woods T. N.
, Astronomy and Astrophysics, Jun, Volume 542, p.L25, (2012)
|
|
Can a halo CME from the limb be geoeffective?,
Cid, C., Cremades H., Aran A., Mandrini C., Sanahuja B., Schmieder B., Menvielle M., Rodriguez L., Saiz E., Cerrato Y., et al.
, Journal of Geophysical Research (Space Physics), Volume 117, p.11102, (2012)
|
|
Outflow Velocity Structure in the Upper Transition Region and Corona,
Gabriel, A., and Abbo L.
, Solar Physics, Volume 280, p.435-443, (2012)
|
