Development and Improvement of the International Reference Ionosphere with special emphasis on the topside and extension to the plasmasphere

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F24%3A00600031" target="_blank" >RIV/68378289:_____/24:00600031 - isvavai.cz</a>

Výsledek na webu

<a href="https://www.annalsofgeophysics.eu/index.php/annals/article/view/9145/7720" target="_blank" >https://www.annalsofgeophysics.eu/index.php/annals/article/view/9145/7720</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.4401/ag-9145" target="_blank" >10.4401/ag-9145</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Development and Improvement of the International Reference Ionosphere with special emphasis on the topside and extension to the plasmasphere

Popis výsledku v původním jazyce

The International Reference Ionosphere is the international standard for Earth’s ionosphere and recognized as such by the International Standardization Organization (ISO), the Committee on Space Research (COSPAR), the International Union of Radio Science (URSI) and many other organizations.nThis paper gives a brief introduction of the IRI model highlighting the many uses of the model in many different fields of theoretical and applied sciences and the ongoing efforts to upgrade the climatological IRI model to real-time conditions with updating indices or by assimilating data into the background IRI. The main part of the paper reviews the recent improvements and evaluations of the IRI topside electron density model and presents a new model option for extending IRI to plasmaspheric altitudes. At the heart of this new option is the use of existing empirical plasmasphere models and the Booker (1977) approach that has so successfully been applied in IRI for modelling the plasma temperatures and ion composition. Three empirical plasmasphere models are evaluated as candidates for this extension option: Carpenter and Anderson (1992), Gallagher et al. (2000), and Ozhogin et al. (2012).

Název v anglickém jazyce

Development and Improvement of the International Reference Ionosphere with special emphasis on the topside and extension to the plasmasphere

Popis výsledku anglicky

The International Reference Ionosphere is the international standard for Earth’s ionosphere and recognized as such by the International Standardization Organization (ISO), the Committee on Space Research (COSPAR), the International Union of Radio Science (URSI) and many other organizations.nThis paper gives a brief introduction of the IRI model highlighting the many uses of the model in many different fields of theoretical and applied sciences and the ongoing efforts to upgrade the climatological IRI model to real-time conditions with updating indices or by assimilating data into the background IRI. The main part of the paper reviews the recent improvements and evaluations of the IRI topside electron density model and presents a new model option for extending IRI to plasmaspheric altitudes. At the heart of this new option is the use of existing empirical plasmasphere models and the Booker (1977) approach that has so successfully been applied in IRI for modelling the plasma temperatures and ion composition. Three empirical plasmasphere models are evaluated as candidates for this extension option: Carpenter and Anderson (1992), Gallagher et al. (2000), and Ozhogin et al. (2012).

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10305 - Fluids and plasma physics (including surface physics)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2024

Kód důvěrnosti údajů

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

Název periodika

Annals of Geophysics

ISSN

1593-5213

e-ISSN

2037-416X

Svazek periodika

67

Číslo periodika v rámci svazku

4

Stát vydavatele periodika

IT - Italská republika

Počet stran výsledku

21

Strana od-do

SA443

Kód UT WoS článku

001407406300016

EID výsledku v databázi Scopus

2-s2.0-85209099386