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Tatiana Niembro Hernandez
Smithsonian Astrophysical ObservatoryMeeting roles in:
Following a Filament Eruption from the Sun to Earth that caused an Intense Geomagnetic Storm
Can We Predict the Solar Wind at Earth Using Parker Solar Probe Measurements?
Advances in Understanding the Innermost Heliosphere I Oral
Energy Flux Contributions and Alfvénic Wave Dynamics in the Inner Heliosphere: Results from Parker Solar Probe Encounters 22–24
Advances in Understanding the Innermost Heliosphere II Oral
Investigating hemispheric asymmetries in coronal hole solar wind structured by magnetolatitude
Direct Measurement of Polar Coronal Hole-like Solar Wind in its Acceleration Phase
Advances in Understanding the Innermost Heliosphere III Oral
Advances in Understanding the Innermost Heliosphere IV Poster
Radial velocity fluctuations at Parker Solar Probe during closest approach in encounter 22
Advances in Understanding the Innermost Heliosphere V Poster
Parker Solar Probe Observations of long-duration high-speed-stream from coronal holes
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