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Solar wind
Example of STEREO Heliospheric Imagery of the solar wind in white light, differential image (the event was discussed here)
Compare ENLIL predictions (modeling) of the behavior of the solar wind parameters based on
- Interplanetary Scintillation (IPS) monitoring (left)
- using solar magnetograph data (right)
![enlil-isee'.png](https://static.wixstatic.com/media/2ef75c_4f38377a34464f119c14cc1e098b2144~mv2.png/v1/fill/w_877,h_465,al_c,q_90,usm_0.66_1.00_0.01,enc_avif,quality_auto/enlil-isee'.png)
Contact Us
If you have any questions or collaboration suggestions, please contact Dr. Olga Khabarova
olgakhabar(at)tauex.tau.ac.il
fax: +972-3-6409282
Department of Geophysics, Faculty of Exact Sciences, Kaplun building.
Tel-Aviv University , P.O.B 39040, Ramat Aviv, 6139001, Tel Aviv 69978
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