The space environment of Mercury at the times of the second and third MESSENGER flybys

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F11%3A00381399" target="_blank" >RIV/68378289:_____/11:00381399 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/67985815:_____/11:00481685

Výsledek na webu

<a href="http://dx.doi.org/10.1016/j.pss.2011.01.018" target="_blank" >http://dx.doi.org/10.1016/j.pss.2011.01.018</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.pss.2011.01.018" target="_blank" >10.1016/j.pss.2011.01.018</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The space environment of Mercury at the times of the second and third MESSENGER flybys

Popis výsledku v původním jazyce

The second and third flybys of Mercury by the MESSENGER spacecraft occurred, respectively, on 6 October 2008 and on 29 September 2009. In order to provide contextual information about the solar wind properties and the interplanetary magnetic field (IMF)near the planet at those times, we have used an empirical modeling technique combined with a numerical physics-based solar wind model. The Wang?Sheeley?Arge (WSA) method uses solar photospheric magnetic field observations (from Earth-based instruments) in order to estimate the inner heliospheric radial flow speed and radial magnetic field out to 21.5 solar radii from the Sun. This information is then used as input to the global numerical magnetohydrodynamic model, ENLIL, which calculates solar wind velocity, density, temperature, and magnetic field strength and polarity throughout the inner heliosphere. WSA-ENLIL calculations are presented for the several-week period encompassing the second and third flybys. This information, in conjunc

Název v anglickém jazyce

The space environment of Mercury at the times of the second and third MESSENGER flybys

Popis výsledku anglicky

The second and third flybys of Mercury by the MESSENGER spacecraft occurred, respectively, on 6 October 2008 and on 29 September 2009. In order to provide contextual information about the solar wind properties and the interplanetary magnetic field (IMF)near the planet at those times, we have used an empirical modeling technique combined with a numerical physics-based solar wind model. The Wang?Sheeley?Arge (WSA) method uses solar photospheric magnetic field observations (from Earth-based instruments) in order to estimate the inner heliospheric radial flow speed and radial magnetic field out to 21.5 solar radii from the Sun. This information is then used as input to the global numerical magnetohydrodynamic model, ENLIL, which calculates solar wind velocity, density, temperature, and magnetic field strength and polarity throughout the inner heliosphere. WSA-ENLIL calculations are presented for the several-week period encompassing the second and third flybys. This information, in conjunc

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BN - Astronomie a nebeská mechanika, astrofyzika

OECD FORD obor

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Projekt

—

Návaznosti

Z - Vyzkumny zamer (s odkazem do CEZ)

Rok uplatnění

2011

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Planetary and Space Science

ISSN

0032-0633

e-ISSN

—

Svazek periodika

59

Číslo periodika v rámci svazku

15

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

9

Strana od-do

2066-2074

Kód UT WoS článku

000298722800023

EID výsledku v databázi Scopus

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