Biblio

Found 38 results

Filters: Author is Schmieder, B. [Clear All Filters]

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)

Dynamics of quiescent prominence fine structures analyzed by 2D non-LTE modelling of the Hα line, Gunár, S., Mein P., Schmieder B., Heinzel P., and Mein N. , Astronomy and Astrophysics, Volume 543, p.A93, (2012)

2011

2D radiative-magnetohydrostatic model of a prominence observed by Hinode, SoHO/SUMER and Meudon/MSDP, Berlicki, A., Gunár S., Heinzel P., Schmieder B., and Schwartz P. , Astronomy and Astrophysics, Jun, Volume 530, p.A143, (2011)

2010

Velocity vectors of a quiescent prominence observed by Hinode/SOT and the MSDP (Meudon), Schmieder, B., Chandra R., Berlicki A., and Mein P. , Astronomy and Astrophysics, Volume 514, p.A68, (2010)

2008

Hinode, TRACE, SOHO, and Ground-based Observations of a Quiescent Prominence, Heinzel, P., Schmieder B., Fárník F., Schwartz P., Labrosse N., Kotrič P., Anzer U., Molodij G., Berlicki A., DeLuca E. E., et al. , Astrophysical Journal, Oct, Volume 686, p.1383-1396, (2008)

On Lyman-line asymmetries in quiescent prominences, Gunár, S., Heinzel P., Anzer U., and Schmieder B. , Astronomy and Astrophysics, Oct, Volume 490, p.307-313, (2008)

2007

Non-LTE Analysis of Lyman-Line Observations of a Filament with SUMER, Schwartz, P., Schmieder B., and Heinzel P. , The Physics of Chromospheric Plasmas, May, Volume 368, p.359, (2007)

Properties of prominence fine-structure threads derived from SOHO/SUMER hydrogen Lyman lines, Gunár, S., Heinzel P., Schmieder B., Schwartz P., and Anzer U. , Astronomy and Astrophysics, Sep, Volume 472, p.929-936, (2007)

Spectral Diagnostics of the Magnetic Field Orientation in a Prominence Observed with SOHO/SUMER, Schmieder, B., Gunár S., Heinzel P., and Anzer U. , Solar Physics, Mar, Volume 241, p.53-66, (2007)

2006

Study of an extended EUV filament using SoHO/SUMER observations of the hydrogen Lyman lines, Schwartz, P., Heinzel P., Schmieder B., and Anzer U. , Astronomy and Astrophysics, Nov, Volume 459, p.651-661, (2006)

2005

Non-LTE diagnostics of velocity fields during the gradual phase of a solar flare, Berlicki, A., Heinzel P., Schmieder B., Mein P., and Mein N. , Astronomy and Astrophysics, Feb, Volume 430, p.679-689, (2005)

Non-Lte Modelling of the EUV Filament Based on Soho/sumer Observations of the Hydrogen Lyman Lines, Schwartz, P., Heinzel P., and Schmieder B. , The Dynamic Sun: Challenges for Theory and Observations, Dec, Volume 600, (2005)

2004

Determination of the 3D structure of an EUV-filament observed by SoHO/CDS, SoHO/SUMER and VTT/MSDP, Schwartz, P., Heinzel P., Anzer U., and Schmieder B. , Astronomy and Astrophysics, Jul, Volume 421, p.323-338, (2004)

Evolution and magnetic topology of the M 1.0 flare of October 22, 2002, Berlicki, A., Schmieder B., Vilmer N., Aulanier G., and Del Zanna G. , Astronomy and Astrophysics, Sep, Volume 423, p.1119-1131, (2004)

Multi-wavelength study of a high-latitude EUV filament, Schmieder, B., Lin Y., Heinzel P., and Schwartz P. , Solar Physics, Jun, Volume 221, p.297-323, (2004)

2003

Determination of the 3D-topology of an EUV-filament observed by SoHO/CDS SoHO/SUMER and VTT/MSDP, Schwartz, P., Heinzel P., Schmieder B., and Anzer U. , Solar Variability as an Input to the Earth's Environment, Sep, Volume 535, p.495-498, (2003)

EUV-filaments and their mass loading, Heinzel, P., Anzer U., Schmieder B., and Schwartz P. , Solar Variability as an Input to the Earth's Environment, Sep, Volume 535, p.447-457, (2003)

Spectroscopic diagnostics of an Hα and EUV filament observed with THEMIS and SOHO, Schmieder, B., Tziotziou K., and Heinzel P. , Astronomy and Astrophysics, Apr, Volume 401, p.361-375, (2003)

A Spectroscopic Model of euv Filaments, Heinzel, P., Anzer U., and Schmieder B. , Solar Physics, Sep, Volume 216, p.159-171, (2003)

2002

The magnetic nature of wide EUV filament channels and their role in the mass loading of CMEs, Aulanier, G., and Schmieder B. , Astronomy and Astrophysics, May, Volume 386, p.1106-1122, (2002)

Spectral diagnostics of the magnetic field orientation in a round-shaped filament, Schmieder, B., Mein N., Heinzel P., and Anzer U. , Solar Variability: From Core to Outer Frontiers, Dec, Volume 506, p.469-472, (2002)

2001

The Relationship between CMEs and Prominence Eruptions, Schmieder, B., van Driel-Gesztelyi L., Delannée C., Simnett G. M., and Wiik J. E. , Recent Insights into the Physics of the Sun and Heliosphere: Highlights from SOHO and Other Space Missions, Volume 203, p.310, (2001)

SOHO/SUMER observations and analysis of the hydrogen Lyman spectrum in solar prominences, Heinzel, P., Schmieder B., Vial J.-C., and Kotrič P. , Astronomy and Astrophysics, Apr, Volume 370, p.281-297, (2001)

Why Are Solar Filaments More Extended in Extreme-Ultraviolet Lines than in Hα?, Heinzel, P., Schmieder B., and Tziotziou K. , Astrophysical Journal Letters, Nov, Volume 561, p.L223-L227, (2001)

2000

Dynamics in Restructuring Active Regions Observed During Soho/Yohkoh/Gbo Campaigns, Schmieder, B., Deng Y., Mandrini C. H., Rudawy P., Nitta N., Mason H., Fletcher L., Martens P., and Brynildsen N. , Advances in Space Research, Volume 25, p.1879-1882, (2000)

Pages