Difference between revisions of "Early warning system (solar radiation)"
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'''Safe'''<br/> | '''Safe'''<br/> | ||
− | <small>Minimal solar activity. | + | <small>Minimal solar activity. Proceed with guarded caution. Have a good day :)</small> |
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<small>'''A possible simple "flag" system to warn colonists of solar radiation levels'''</small> | <small>'''A possible simple "flag" system to warn colonists of solar radiation levels'''</small> | ||
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Instruments in the Earth-Sun <math>L_1</math> point already provide scientists on Earth with an '''early warning system''' to monitor [[:category:Space Weather|space weather]]. Probes such as ''SoHO'' and ''ACE'' receive solar ions approximately an hour before they impact the Earth's atmosphere.<ref>[http://www.astroengine.net/projects.php#svalbard Project: ''Solar Wind – Magnetospheric Interaction: Magnetic Storms and the Aurora'' (page 16), Ian J. O'Neill and Gareth P. Thomas, University Center on Svalbard (UNIS), April 2002]</ref> This not only provides excellent diagnostic data, but also gives advanced warning to companies and organizations that the Earth is 60 minutes away from experiencing an increase in [[solar radiation]]. Emergency procedures can be enacted accordingly, possibly saving delicate satellites and astronauts. | Instruments in the Earth-Sun <math>L_1</math> point already provide scientists on Earth with an '''early warning system''' to monitor [[:category:Space Weather|space weather]]. Probes such as ''SoHO'' and ''ACE'' receive solar ions approximately an hour before they impact the Earth's atmosphere.<ref>[http://www.astroengine.net/projects.php#svalbard Project: ''Solar Wind – Magnetospheric Interaction: Magnetic Storms and the Aurora'' (page 16), Ian J. O'Neill and Gareth P. Thomas, University Center on Svalbard (UNIS), April 2002]</ref> This not only provides excellent diagnostic data, but also gives advanced warning to companies and organizations that the Earth is 60 minutes away from experiencing an increase in [[solar radiation]]. Emergency procedures can be enacted accordingly, possibly saving delicate satellites and astronauts. | ||
− | A simple, cost effective probe may be inserted into the Mars-Sun <math>L_1</math> point. This probe needn't be as sophisticated as ''SoHO'' or ''ACE'', it just needs to monitor the flux of energetic particles | + | A simple, cost effective probe may be inserted into the Mars-Sun <math>L_1</math> point. This probe needn't be as sophisticated as ''SoHO'' or ''ACE'', it just needs to monitor the flux of energetic particles traveling toward Mars. Akin to a "flag" system on a patrolled beach (red for "dangerous", no swimming. Green for "safe", water is safe), Mars settlers could have advanced warning of an incoming [[CME]] from the Sun. If constantly measured by a particle detector on the probe at the <math>L_1</math> point, various stages of danger levels may be used to indicate to settlers unprotected on the surface of what severity of risk they are in. Surface "walkabouts" may be tightly restricted by such a system. |
==Outstanding design issues== | ==Outstanding design issues== | ||
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The distance between Earth's <math>L_1</math> point (with the probes measuring solar particles) and the planet is approximately 1.5 million km. This provides information on the solar wind particles approximately 1 hour before they are received on Earth. Mars is a less massive planet than the Earth, therefore, Mars' <math>L_1</math> point will be closer to the planet than the Earth's. | The distance between Earth's <math>L_1</math> point (with the probes measuring solar particles) and the planet is approximately 1.5 million km. This provides information on the solar wind particles approximately 1 hour before they are received on Earth. Mars is a less massive planet than the Earth, therefore, Mars' <math>L_1</math> point will be closer to the planet than the Earth's. | ||
− | Reaching a logical conclusion, assuming solar particles are | + | Reaching a logical conclusion, assuming solar particles are traveling at the same velocity in near-Mars orbit as with near-Earth orbit, a Mars early warning system of the design outlined above will be less effective than the terrestrial version. So, how much time will the Mars early warning system provide to colonists from detection (at <math>L_1</math>) to impact (at Mars' surface)? |
Using the equation from [[Lagrangian point]] calculations: | Using the equation from [[Lagrangian point]] calculations: | ||
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<references/> | <references/> | ||
− | [[category: | + | [[category:Radiation Protection]] |
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Latest revision as of 16:09, 17 December 2018
Like Earth, Mars has its own Lagrangian points with the Sun. Currently there are no man-made satellites in or orbit, but it is conceivable that these islands of gravitational stability may be used to greatly benefit future Mars colonies.
Contents
Early warning system for the onset of solar storms
Danger |
Caution |
Safe |
A possible simple "flag" system to warn colonists of solar radiation levels
Instruments in the Earth-Sun point already provide scientists on Earth with an early warning system to monitor space weather. Probes such as SoHO and ACE receive solar ions approximately an hour before they impact the Earth's atmosphere.[1] This not only provides excellent diagnostic data, but also gives advanced warning to companies and organizations that the Earth is 60 minutes away from experiencing an increase in solar radiation. Emergency procedures can be enacted accordingly, possibly saving delicate satellites and astronauts.
A simple, cost effective probe may be inserted into the Mars-Sun point. This probe needn't be as sophisticated as SoHO or ACE, it just needs to monitor the flux of energetic particles traveling toward Mars. Akin to a "flag" system on a patrolled beach (red for "dangerous", no swimming. Green for "safe", water is safe), Mars settlers could have advanced warning of an incoming CME from the Sun. If constantly measured by a particle detector on the probe at the point, various stages of danger levels may be used to indicate to settlers unprotected on the surface of what severity of risk they are in. Surface "walkabouts" may be tightly restricted by such a system.
Outstanding design issues
The Mars time lag problem?
The distance between Earth's point (with the probes measuring solar particles) and the planet is approximately 1.5 million km. This provides information on the solar wind particles approximately 1 hour before they are received on Earth. Mars is a less massive planet than the Earth, therefore, Mars' point will be closer to the planet than the Earth's.
Reaching a logical conclusion, assuming solar particles are traveling at the same velocity in near-Mars orbit as with near-Earth orbit, a Mars early warning system of the design outlined above will be less effective than the terrestrial version. So, how much time will the Mars early warning system provide to colonists from detection (at ) to impact (at Mars' surface)?
Using the equation from Lagrangian point calculations:
where is the distance of from Mars, is the distance between the bodies and and are the masses of Mars and the Sun respectively.
Using R = 2.28 × 1011 meters, MM = 6.4191×1023 kg and MS = 1.98892×1030 kg, we arrive at a value of:
- meters or 1.08 million km, 72% of the distance of Earth's 1.5 million km.
Now, keeping the assumption that it will approximately take solar ions 60 minutes to travel 1.5 million km (from Earth's point to Earth), the time from to Mars' surface = 60 × 72% = 43.2 minutes.
Although 43 minutes is less than the warning time Earth-based solar wind probes are able to provide, this is not a great reduction in lag time, and would still greatly benefit the humans unprotected from solar radiation.