Biblio
Found 43 results
Filters: Author is Schmieder, B. [Clear All Filters]
Low Geo-Effectiveness of Fast Halo CMEs Related to the 12 X-Class Flares in 2002,
, Journal of Geophysical Research (Space Physics), Volume 125, p.e27529, (2020)
Role of the Coronal Environment in the Formation of Four Shocks Observed without Coronal Mass Ejections at Earth's Lagrangian Point L1,
, Astrophys. J., Volume 895, p.144, (2020)
Time Evolution of the Altitude of an Observed Coronal Wave,
, Solar Physics, Volume 289, Issue 7, p.2565-2585, (2014)
Can a halo CME from the limb be geoeffective?,
, 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,
, Astronomy and Astrophysics, Volume 543, p.A93, (2012)
2D radiative-magnetohydrostatic model of a prominence observed by Hinode, SoHO/SUMER and Meudon/MSDP,
, Astronomy and Astrophysics, Jun, Volume 530, p.A143, (2011)
Velocity vectors of a quiescent prominence observed by Hinode/SOT and the MSDP (Meudon),
, Astronomy and Astrophysics, Volume 514, p.A68, (2010)
Hinode, TRACE, SOHO, and Ground-based Observations of a Quiescent Prominence,
, Astrophysical Journal, Oct, Volume 686, p.1383-1396, (2008)
On Lyman-line asymmetries in quiescent prominences,
, Astronomy and Astrophysics, Oct, Volume 490, p.307-313, (2008)
Non-LTE Analysis of Lyman-Line Observations of a Filament with SUMER,
, The Physics of Chromospheric Plasmas, May, Volume 368, p.359, (2007)
Properties of prominence fine-structure threads derived from SOHO/SUMER hydrogen Lyman lines,
, Astronomy and Astrophysics, Sep, Volume 472, p.929-936, (2007)
Spectral Diagnostics of the Magnetic Field Orientation in a Prominence Observed with SOHO/SUMER,
, Solar Physics, Mar, Volume 241, p.53-66, (2007)
Study of an extended EUV filament using SoHO/SUMER observations of the hydrogen Lyman lines,
, Astronomy and Astrophysics, Nov, Volume 459, p.651-661, (2006)
Non-LTE diagnostics of velocity fields during the gradual phase of a solar flare,
, 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,
, The Dynamic Sun: Challenges for Theory and Observations, Dec, Volume 600, (2005)
Determination of the 3D structure of an EUV-filament observed by SoHO/CDS, SoHO/SUMER and VTT/MSDP,
, Astronomy and Astrophysics, Jul, Volume 421, p.323-338, (2004)
Evolution and magnetic topology of the M 1.0 flare of October 22, 2002,
, Astronomy and Astrophysics, Sep, Volume 423, p.1119-1131, (2004)
Multi-wavelength study of a high-latitude EUV filament,
, Solar Physics, Jun, Volume 221, p.297-323, (2004)
Determination of the 3D-topology of an EUV-filament observed by SoHO/CDS SoHO/SUMER and VTT/MSDP,
, Solar Variability as an Input to the Earth's Environment, Sep, Volume 535, p.495-498, (2003)
EUV-filaments and their mass loading,
, 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,
, Astronomy and Astrophysics, Apr, Volume 401, p.361-375, (2003)
A Spectroscopic Model of euv Filaments,
, Solar Physics, Sep, Volume 216, p.159-171, (2003)
The magnetic nature of wide EUV filament channels and their role in the mass loading of CMEs,
, Astronomy and Astrophysics, May, Volume 386, p.1106-1122, (2002)