<span style="font-size: x-small; font-family: times new roman,times;"><span style="line-height: 115%; mso-fareast-font-family: Calibri; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA;" lang="EN-US">An updated model of O<sup>+</sup>(<sup>2</sup>P) 7320 Å dayglow emission</span></span>
Online Publishing @ NISCAIR
View Archive InfoField | Value | |
Authentication Code |
dc |
|
Title Statement |
<span style="font-size: x-small; font-family: times new roman,times;"><span style="line-height: 115%; mso-fareast-font-family: Calibri; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA;" lang="EN-US">An updated model of O<sup>+</sup>(<sup>2</sup>P) 7320 Å dayglow emission</span></span> |
|
Added Entry - Uncontrolled Name |
Thirupathaiah, P ; Indian Institute of Technology Roorkee Dharwan, Maneesha ; Indian Institute of Technology Roorkee Singh, Vir ; Indian Institute of Technology Roorkee |
|
Uncontrolled Index Term |
Airglow emission, solar EUV radiation flux, O+(2P) 7320 Å dayglow emission, volume emission rate |
|
Summary, etc. |
<span style="font-size: 12pt; font-family: "Times New Roman","serif"; line-height: 115%; mso-fareast-font-family: Calibri; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: AR-SA;" lang="EN-US">A comprehensive model is developed using the updated rate coefficients and transition probabilities to study the O<sup>+</sup>(<sup>2</sup>P) 7320 Å dayglow emission. The solar EUV fluxes calculated using the Solar Irradiance Platform (SIP) are incorporated into the model. The neutral atmospheric parameters are adopted from the NRLMSISE-00 model. The ionospheric parameters are adopted from the IRI-07 model. The measurements as provided by instruments onboard Atmosphere Explorer-C satellite, Dynamics Explorer-2 spacecraft and Upper Atmosphere Research Satellite are used to validate the model results. It has been found that the emission rates computed using the present model are in good agreement with the measurements. It is also found that the present model results are in better agreement with the measurements in comparison with the earlier models. The model results show that the updated rate coefficients and transition probabilities are quite consistent with each other and may be used in the aeronomical studies.</span> |
|
Publication, Distribution, Etc. |
Indian Journal of Radio & Space Physics (IJRSP) 2017-01-04 10:12:43 |
|
Electronic Location and Access |
application/pdf http://op.niscair.res.in/index.php/IJRSP/article/view/6557 |
|
Data Source Entry |
Indian Journal of Radio & Space Physics (IJRSP); ##issue.vol## 44, ##issue.no## 1 (2015): Indian Journal of Radio & Space Physics |
|
Language Note |
en |
|
Nonspecific Relationship Entry |
http://op.niscair.res.in/index.php/IJRSP/article/download/6557/16725 http://op.niscair.res.in/index.php/IJRSP/article/download/6557/16726 |
|
Terms Governing Use and Reproduction Note |
Except where otherwise noted, the Articles on this site are licensed underCreative Commons License: CC Attribution-Noncommercial-No Derivative Works 2.5 India© 2012. The Council of Scientific & Industrial Research, New Delhi. |
|