Difference between revisions of "Solar Flares"
Cholmondely (talk | contribs) (Page Created) |
Cholmondely (talk | contribs) (Added Cody's screen shots & gubbins from Wikipedia) |
||
| Line 1: | Line 1: | ||
A simple OXP that adds some flavour to systems that have "solar activity". The corona flare value of the sun occasionally increases, and then returns back to normal after a short period of time. | A simple OXP that adds some flavour to systems that have "solar activity". The corona flare value of the sun occasionally increases, and then returns back to normal after a short period of time. | ||
| + | [[File:Solar Flares OXP Normal.png|right|thumb|Normal Activity]] | ||
| + | [[File:Solar Flares OXP Flare.png|right|thumb|Flaring]] | ||
| + | |||
| + | == From Wikipedia == | ||
| + | [[File:Magnificent CME Erupts on the Sun - August 31.jpg|thumb|320px|left|Solar Flare (coronal mass ejection)]] | ||
| + | A solar flare is a sudden flash of increased brightness on the Sun, usually observed near its surface and in close proximity to a sunspot group. Powerful flares are often, but not always, accompanied by a coronal mass ejection. Even the most powerful flares are barely detectable in the total solar irradiance (the "solar constant"). | ||
| + | |||
| + | Solar flares occur in a power-law spectrum of magnitudes; an energy release of typically 1020 joules of energy suffices to produce a clearly observable event, while a major event can emit up to 1025 joules. | ||
| + | |||
| + | Flares are closely associated with the ejection of plasmas and particles through the Sun's corona into outer space; flares also copiously emit radio waves. If the ejection is in the direction of the Earth, particles associated with this disturbance can penetrate into the upper atmosphere (the ionosphere) and cause bright auroras, and may even disrupt long range radio communication. It usually takes days for the solar plasma ejecta to reach Earth. Flares also occur on other stars, where the term stellar flare applies. High-energy particles, which may be relativistic, can arrive almost simultaneously with the electromagnetic radiations. | ||
| + | <div style="clear:both"></div> | ||
== Licence == | == Licence == | ||
Revision as of 23:01, 6 May 2021
A simple OXP that adds some flavour to systems that have "solar activity". The corona flare value of the sun occasionally increases, and then returns back to normal after a short period of time.
Contents
From Wikipedia
A solar flare is a sudden flash of increased brightness on the Sun, usually observed near its surface and in close proximity to a sunspot group. Powerful flares are often, but not always, accompanied by a coronal mass ejection. Even the most powerful flares are barely detectable in the total solar irradiance (the "solar constant").
Solar flares occur in a power-law spectrum of magnitudes; an energy release of typically 1020 joules of energy suffices to produce a clearly observable event, while a major event can emit up to 1025 joules.
Flares are closely associated with the ejection of plasmas and particles through the Sun's corona into outer space; flares also copiously emit radio waves. If the ejection is in the direction of the Earth, particles associated with this disturbance can penetrate into the upper atmosphere (the ionosphere) and cause bright auroras, and may even disrupt long range radio communication. It usually takes days for the solar plasma ejecta to reach Earth. Flares also occur on other stars, where the term stellar flare applies. High-energy particles, which may be relativistic, can arrive almost simultaneously with the electromagnetic radiations.
Licence
This work is licensed under the Creative Commons Attribution-Noncommercial-Share Alike 4.0 Unported License. To view a copy of this license, visit http://creativecommons.org/licenses/by-nc-sa/4.0/
Code borrowed from the the "Nova Mission" code in the code Oolite application. Copyright © 2004-2018 Giles C Williams and contributors
This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or (at your option) any later version. To view information about this licence, visit https://www.gnu.org/licenses/old-licenses/gpl-2.0.en.html
Version History
- 1.1
- System corona hue and flare values should now be restored correctly after a save game, so when the system is left no changes will be stored.
- 1.0
- Initial release.
Downloads
Downloadable through the in-game Expansions Manager
Links
Gameplay and Balance indicator
