Pre-release of the source code for Palumbo et al. (in prep.) - "Characterizing Solar Center-to-limb Radial-velocity Variability with SDO" Full Changelog: https://github.com/palumbom/sdo-clv-pipeline/commits/v0.1.0If you use this software, please cite it using the metadata from this file
Presentation of a Solar Mission to ESA: The EUV Variability Experiment (EVE) on the Solar Dynamics O...
Context. Observations from the Solar Dynamics Observatory (SDO) have the potential for allowing the ...
This volume is dedicated to the Solar Dynamics Observatory (SDO), which was launched 11 February 201...
This record contains the output generated by sdo-clv-pipeline for use in Palumbo et al. (in prep.) -...
We estimate disc-averaged radial-velocity variations, unsigned magnetic flux and active-region filli...
Context. It is possible to detect and track coronal bright points (CBPs) in Solar Dynamics Observato...
The Helioseismic and Magnetic Imager of SDO will provide uninterrupted 4k x 4k-pixel Doppler-shift i...
Context. The measurement of the Sun’s surface motions with a high spatial and temporal res...
In recent years, the search for Earth-mass planets using radial-velocity measurements has become inc...
International audienceThis paper presents SOAP 2.0, a new version of the Spot Oscillation And Planet...
International audienceIn Fall 2008 NASA selected a large international consortium to produce a compr...
This presentation focuses on the first space weather research mission in the Living with a Star (LWS...
This pre-release of the cosmo-tools contains a set of tools developed during the COSMO project (CTM2...
SDO’s unprecedented data volume poses an entirely new set of challenges with respect to data access,...
The High Resolution Echelle Spectrograph (HIRES) at the W.M. Keck Observatory (WMKO) is one of the m...
Presentation of a Solar Mission to ESA: The EUV Variability Experiment (EVE) on the Solar Dynamics O...
Context. Observations from the Solar Dynamics Observatory (SDO) have the potential for allowing the ...
This volume is dedicated to the Solar Dynamics Observatory (SDO), which was launched 11 February 201...
This record contains the output generated by sdo-clv-pipeline for use in Palumbo et al. (in prep.) -...
We estimate disc-averaged radial-velocity variations, unsigned magnetic flux and active-region filli...
Context. It is possible to detect and track coronal bright points (CBPs) in Solar Dynamics Observato...
The Helioseismic and Magnetic Imager of SDO will provide uninterrupted 4k x 4k-pixel Doppler-shift i...
Context. The measurement of the Sun’s surface motions with a high spatial and temporal res...
In recent years, the search for Earth-mass planets using radial-velocity measurements has become inc...
International audienceThis paper presents SOAP 2.0, a new version of the Spot Oscillation And Planet...
International audienceIn Fall 2008 NASA selected a large international consortium to produce a compr...
This presentation focuses on the first space weather research mission in the Living with a Star (LWS...
This pre-release of the cosmo-tools contains a set of tools developed during the COSMO project (CTM2...
SDO’s unprecedented data volume poses an entirely new set of challenges with respect to data access,...
The High Resolution Echelle Spectrograph (HIRES) at the W.M. Keck Observatory (WMKO) is one of the m...
Presentation of a Solar Mission to ESA: The EUV Variability Experiment (EVE) on the Solar Dynamics O...
Context. Observations from the Solar Dynamics Observatory (SDO) have the potential for allowing the ...
This volume is dedicated to the Solar Dynamics Observatory (SDO), which was launched 11 February 201...
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