TN
Member Since 2011
Tatiana Niembro Hernandez
Astrophysicist, Smithsonian Astrophysical Observatory
AGU Research
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Parker Solar Probe observations of coronal holes originated long-duration high-speed-streams
UNDERSTANDING THE ORIGINS AND EVOLUTION OF LARGE-SCALE STRUCTURES IN THE HELIOSPHERE WITH OBSERVATIONS AND MODELING II POSTER
spa-solar and heliospheric physics | 13 december 2024
Nishu Karna, Tatiana Niembro Hernandez
The solar wind originating from different solar source regions has distinct plasma and magnetic field properties and propagates at different velocitie...
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ParkerSolarWind - a Python code for 1D Parker solar wind solutions
INNOVATIVE PYTHON SOFTWARE IN SOLAR AND SPACE PHYSICS POSTER
spa-magnetospheric physics | 12 december 2024
Samuel T. Badman, Lidiya Y. Ahmed, Jean-Baptiste ...
One of the seminal models in heliophysics is the Parker solution of the expanding solar wind (Parker 1958,1960). While the governing physics and equat...
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Structures Within Coronal Mass Ejections Associated to Large Events of Geomagnetic Activity
DOWN TO EARTH WITH SPACE WEATHER: MAGNETIC STORM–INDUCED GEOELECTRIC FIELDS, CURRENTS, AND IMPACTS I POSTER
geomagnetism, paleomagnetism and electromagnetism | 12 december 2024
Sergio Vidal-Luengo, Tatiana Niembro Hernandez, De...
It has been widely noticed that large solar wind structures can induce significant ground magnetic field responses on Earth, which in turn can generat...
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Kinetic complexities of the near-Sun heliospheric current sheet observed by Parker Solar Probe
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA VI POSTER
spa-solar and heliospheric physics | 11 december 2024
Jaye Verniero, Kristoff W. Paulson, Adam Szabo, Ol...
The heliospheric current sheet (HCS), which separates the Suns magnetic field lines of opposite polarity in the solar wind, is a complex structure tha...
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How Important is Solar Latitude in Tracking the Solar Wind?
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA V POSTER
spa-solar and heliospheric physics | 11 december 2024
Penelope Planet, Samuel T. Badman, Michael L. Ste...
The solar wind is an intrinsically three-dimensional structure whose full complexity needs to be understood to accurately model and predict space weat...
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The May 2024 Interplanetary Coronal Mass Ejections Observed by HAWC
COSMIC RAY TRANSPORT: PARKER SOLAR PROBE AND SOLAR ORBITER BRIDGING OUTER HELIOSPHERE WITH SOLAR ATMOSPHERE POSTER
spa-solar and heliospheric physics | 10 december 2024
Alejandro Lara, K. P. Arunbabu, Tatiana Niembro He...
In May 2024 the large Active Region 13664 produced a series of X-class flares and several halo coronal mass ejections which reached the Earth vicinity...
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Characterizing the complexity of compression regions related to shocks and their relationship with geomagnetic storms
COLLISIONLESS SHOCKS IN HELIOSPHERIC AND ASTROPHYSICAL PLASMAS AND THEIR EFFECTS ON PLANETARY MAGNETOSPHERES I POSTER
spa-solar and heliospheric physics | 10 december 2024
Tatiana Niembro Hernandez, Alejandro Lara, Sergio ...
It is widely-held belief that major geomagnetic storms (GS) are caused by strong interplanetary shocks. However, some GSs are events with weak or with...
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Study of Intense Geomagnetic Storms that occurred in the Solar Cycles 23 and 24
ADVANCING FUNDAMENTAL SPACE WEATHER RESEARCH: FLARES, CMES, SOLAR WIND, AND EARTH/PLANETARY IMPACTS I POSTER
spa-solar and heliospheric physics | 09 december 2024
Roberto Panuco, Tatiana Niembro Hernandez, Nishu K...
The prediction of Intense Geomagnetic Storms (IGS) that could knock down communications and important infrastructure is a milestone in the study of so...
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