It looks like you're using an Ad Blocker.
Please white-list or disable AboveTopSecret.com in your ad-blocking tool.
Thank you.
Some features of ATS will be disabled while you continue to use an ad-blocker.
You even provided a definition of "major flare," although not all of your sources seem to be using that definition. They also tend to use expressions like "large" in a subjective, comparative fashion. Most solar flare research has focussed on the interaction of the Sun on the Earth's atmosphere and magnetosphere with an eye on their effects on communication. A solar flare that is highly disruptive of the ionosphere, and hence, radio communication may be considered "large" by such a researcher, although it may have no proton flux and be considered as "mild" by someone concerned with astronaut safety.
During the last 6 hours, it has produced three major solar flares. The most intense in x-rays as a class X1.2 event at 00:43 UTC on 15 January. However, this flare was weak compared to the punch produced several hours later by a long-duration class M8.6 event at 06:38 UTC. The M8.6 event is shown in an x-ray image taken by the SXI instrument on the GOES spacecraft:
This long-duration major flare accelerated energetic protons that reached the Earth in less than two hours which have the potential to increase radiation levels in space where spacecraft operate (no danger exists to humans on Earth).
As a result, we selected 166 proton events that were associated with major flares; 85 events associated with X-class flares and 81 events associated with M-class flares.
The X-ray solar flares are classified according to their X-ray brightness in the wavelength range 1 to 8 Å. This brightness is measured as the peak intensity of the burst by the GOES satellites.
• X-class flares have intensities greater than or equal to 10-4 W/m². These events that can trigger planet-wide radio blackouts and long-lasting radiation storms.
• M-class flares have intensities greater than or equal to 10-5 W/m² and lower than 10-4 W/m². They can cause brief radio blackouts especially in the Earth's polar regions.
• C-class flares have intensities greater than or equal to 10-6 W/m² and lower than 10-5 W/m². They have few noticeable consequences on Earth.
The optical solar flares are classified according to their solid angle at the time of maximum brightness in H-alpha (at the wavelength of 656.3 nm).
• a class 4 flare has a solid angle greater than or equal to 24.8 square degrees
• a class 3 flare has a solid angle in the range 12.5 to 24.7 square degrees
• a class 2 flare has a solid angle in the range 5.2 to 12.4 square degrees
• a class 1 flare has a solid angle in the range 2.1 to 5.1 square degrees
• a class 0 flare has a solid angle lower than or equal to 2.0 square degrees
The class is usually followed by a brightness qualifier F (Faint), N (Normal), or B (Brilliant).
The proton belts contain protons with kinetic energies ranging from about 100 keV (which can penetrate 0.6 mm (0.23 inches) of lead) to over 400 MeV (which can penetrate 143 mm (5.62 inches) of lead)
The CM was a conical pressure vessel with a maximum diameter of 3.9 m at its base and a height of 3.65 m. It was made of an aluminum honeycomb sandwhich bonded between sheet aluminum alloy. The base of the CM consisted of a heat shield made of brazed stainless steel honeycomb filled with a phenolic epoxy resin as an ablative material and varied in thickness from 1.8 to 6.9 cm.
Flares release energy in many forms – electromagnetic (gamma rays and X-rays), energetic particles (protons and electrons), and mass flows.
The one of interest here is entitled "Problems in Radiation Shielding of Space Vehicles"
co-authored by Keller, Shelton, Burrell and Downey, four NASA experts. On page 244 they
describe the problem, "Space explorers will be concerned with great radiation belts upon
leaving the Earth, with the background of cosmic radiation that pervades all space, with the
violent particle radiation storms associated with solar activity, and with the radiation belts
around planets to be visited."
On page 253, a chart lists the shielding effects from various materials. I was surprised to
see that water is one of the more effective shields. The chart shows the various amounts of
material necessary to stop the primary protons at their different energy levels. Their chart
shows that stopping a 10 MEV (million electron volts) particle requires 10 cm of water, for a
25 MEV particle you need 25 cm of water, and a 50 MEV event seems to call for 90 cm. The
first two are not very energetic particles because the Sun emits particles of several BEV
(billion electron volts). By contrast, a working atomic reactor emits particles in the 18
MEV range.
On page 256 of Astronautical Engineering and Science, there is a chart that shows the
dosage of four different flares. On August 22, 1958 there was a low energy flare that could
have been reduced to 25 rem per hour with 2 cm of water shielding. On May 10, 1960 there
was high flux, low energy flare that would have needed over 36 cm of water to reduce it to
25 rem per hour. There was an intermediate energy flare on November 12, 1960 and it would
have required 18 cm of shielding to reduce it to the 25 rem per hour. A high energy event
happened on February 23, 1956 which would have required over 35 cm (12-inches) of
shielding water to bring it down to 25 rem per hour.
McKinnon, the governments own expert, telling us: "A probability
of 10-20% should be considered a low probability for class M events, ..." Only a large flare
can be a class M which a medium X-ray emitter event. He also says that at least 1 % will be
the deadliest of solar storms, Class X.
there is complete list of the flares for 25 years.
The total number of flares for the period is 134,793. This averages out to 5,391 flares
per year or 14.76 per day. The Apollo astros... spent a total of 85 days in space. Thus
during that period of time the average number of flares that could be expected was 1254. If
we use... the monthly totals for these same periods of time, we find the total to be 1485 flares.
This increase is expected because the trips took place at the high end of that solar cycle.
To send all these missions to the Moon without reporting severe radiation problems,
NASA is effectively telling us is that not one flare emitted heavy X-Rays or protons during
this time period. But McKinnon's probability of 1 % would mean, at least, 13 super deadly
flares of X rated capacity or over one per mission. In addition they should have been exposed
to 268 M class (medium) flares which is 1/5 of the total number. M class flares are also
deadly without the 2 meters of shielding. Referring again to the chart on p. 256 of
Astronautical Engineering... we see that any hull of one cm thickness would have allowed
70,000 rem for each intermediate flare into the module and many times more from an X-
rated flare.
Mauldin states: "Cosmic particles are dangerous, come from all sides, and require at least
2 meters of solid shielding around all living organisms." "Solar (or star) flares of protons, an
occasional and severe hazard on the way out of and into planetary systems, can give doses of
hundreds to thousands of rem over a few hours at the distance of Earth. Such doses are fatal
and millions of times greater than the permitted dose. Death is likely after 500 rems in any
short time, . . . "
Apollo 10 -05/18 to 05/26 1969 days in space= 8 X-class flares = 2 M-class flares = 11
Apollo 11 -07/16 to 07/24 1969 days in space= 8 X-class flares = 1 M-class flares = 7
Apollo 12 -11/14 to 11/24 1969 days in space= 10 X-class flares = 12 M-class flares = 12
Apollo 13 -04/11 to 04/17 1970 days in space= 6 X-class flares = 1 M-class flares = 10
Apollo 14 -01/31 to 02/09 1971 days in space= 10 X-class flares = 0 M-class flares = 9
Apollo 15 -07/26 to 08/07 1971 days in space= 12 X-class flares = 0 M-class flares = 7
Apollo 16 -04/16 to 04/27 1972 days in space= 13 X-class flares = 0 M-class flares = 2
Apollo 17 -12/07 to 12/19 1972 days in space= 12 X-class flares = 1 M-class flares = 5
The extraordinary solar storms between 18 October 2003 and 5 November 2003 include over 140 flares,primarily from two different large sunspot groups. There were 11 large X-class flares during this period, including an X17 flare on 28 October 2003 and an X28 flare on4 November 2003
You may have said it but you did not provide any source showing that a Class 1 optical flare will produce 500MeV particles.
As I just earlier stated, even a Class 1 flare can have energetic particles up to 500Mev. So any flare, Class 1 and up, can be dangerous to even shielded astronauts.
But energetic proton flux is not the only danger from the flare.
www.newscientist.com...
Smith says that because there would be no warning, the X-ray threat should not be ignored. He suggests that astronauts be given protective aluminium shields to carry with them when they roam far from base.
Please provide a source for 10 to 30 flares per day for Apollo missions. But why do you say 20% of flares produce proton events when your own source says this:
Point is, per day there were between 10 to 30 flares identified during Apollo missions. If go by 10 flares a day and if say 20% of those emitted proton events that would still leave at least 2 flares a day to account for.
www.fin.ucar.edu...
We found that about only 3.5% (1.9% for M-class and 21.3% for X-class) of the flares are associated with the proton events.
“I can stand brute force, but brute reason is quite unbearable. There is something unfair about its use. It is hitting below the intellect.” - Oscar Wilde
www.fin.ucar.edu...
Originally posted by Phage
reply to post by FoosM
You may have said it but you did not provide any source showing that a Class 1 optical flare will produce 500MeV particles.
As I just earlier stated, even a Class 1 flare can have energetic particles up to 500Mev. So any flare, Class 1 and up, can be dangerous to even shielded astronauts.
Right. The levels of electromagnetic radiation emitted during solar flares are easily shielded against. As the article you found concerning long term exposure on the Moon pointed out. The skin of the spacecraft was entirely adequate.
But energetic proton flux is not the only danger from the flare.
www.newscientist.com...
Smith says that because there would be no warning, the X-ray threat should not be ignored. He suggests that astronauts be given protective aluminium shields to carry with them when they roam far from base.
Please provide a source for 10 to 30 flares per day for Apollo missions. But why do you say 20% of flares produce proton events when your own source says this:
Point is, per day there were between 10 to 30 flares identified during Apollo missions. If go by 10 flares a day and if say 20% of those emitted proton events that would still leave at least 2 flares a day to account for.
We found that about only 3.5% (1.9% for M-class and 21.3% for X-class) of the flares are associated with the proton events.
Point is, per day there were between 10 to 30 flares identified during Apollo missions. If go by 10 flares a day and if say 20% of those emitted proton events that would still leave at least 2 flares a day to account for.
Originally posted by Phage
The levels of electromagnetic radiation emitted during solar flares are easily shielded against. The skin of the spacecraft was entirely adequate.
Originally posted by ppk55
Originally posted by Phage
The levels of electromagnetic radiation emitted during solar flares are easily shielded against. The skin of the spacecraft was entirely adequate.
Hello, can you comment on Eleanor Blakely's statement from Jarrah's video that aluminium shielding would cause particles to fragment, and rather than shielding it would exacerbate the problem.
Her section starts at 1.15.
[SPAM LINK DELETED]
Also, here is her CV.
hacd.jsc.nasa.gov...
Originally posted by CHRLZ
Originally posted by Exuberant1
Your arguments are quite sound and would be better if they did not contain insults. It is a pity you could not go back and edit them all out, as this thread would be an excellent research resource without them. Alas.
Exuberant won't see this (the 'champion of debate' has me blocked..) but I would URGE the other members here to make exuberant responsible for his words. He should be asked to back up his very clear inference that many or all of Pinke's arguments contain insults.
If he cannot back that up, he should have the cojones to admit he was wrong, and APOLOGISE.
Apollo 12 was the sixth manned flight in the United States Apollo program and the second to land on the Moon (a H type mission). It was launched on November 14, 1969, four months after Apollo 11. Mission commander Charles "Pete" Conrad and Lunar Module Pilot Alan L. Bean performed just over one day and seven hours of lunar surface activity while Command Module Pilot Richard F Gordon remained in lunar orbit. The landing site for the mission was the Ocean of Storms.
The records also show that no major solar flares occurred during the Apollo missions,
Apollo 12 launched on schedule from Kennedy Space Center, during a rainstorm. It was the first rocket launch attended by an incumbent US president, Richard Nixon. Thirty-six-and-a-half seconds after lift-off, the vehicle triggered a lightning discharge through itself and down to the earth through the Saturn's ionized plume. Protective circuits on the fuel cells in the service module falsely detected overloads and took all three fuel cells offline, along with much of the CSM instrumentation. A second strike at 52 seconds after launch knocked out the "8-ball" attitude indicator. The telemetry stream at Mission Control was garbled nonsense. However, the Saturn V continued to fly correctly; the strikes had not affected the Saturn V's Instrument Unit.
Legendary EECOM John Aaron (the original NASA "steely eyed missile man")[2]remembered the telemetry failure pattern from an earlier test when a power supply malfunctioned in the CSM Signal Conditioning Equipment (SCE)
Aaron made a call: "Try SCE to aux". This switched the SCE to a backup power supply. The switch was fairly obscure and neither the Flight Director, CAPCOM, nor Commander Conrad immediately recognized it. Lunar module pilot Alan Bean, flying in the right seat as the CSM systems engineer, remembered the SCE switch from a training incident a year earlier whenthe same failure had been simulated
. Aaron's quick thinking and Bean's memory saved what could have been an aborted mission.
CAPE CANAVERAL, Fla. – The lightning that thwarted today's planned launch of the space shuttle Endeavour is a familiar problem for NASA's shuttle fleet.
NASA called a 24-hour delay to Endeavour's scheduled STS-127 lift off to investigate possible damage after a powerful electrical storm hit yesterday and 11 lightning bolts impacted Launch Pad 39A here at the seaside Kennedy Space Center.
The Florida coast is often the victim of lightning, as frequent thunderstorms and even hurricanes come in from the ocean on the East. If lightning does occur nearby, the giant metal space shuttle standing tall atop its launch pad tends to attract the brunt of it.
In 2006 the space shuttle Atlantis postponed its STS-115 flight after a powerful lightning bolt impacted with a current of 100,000 amps – the strongest lightning strike yet.
And lightning isn't just a risk while the vehicles sit at the pad; If lightning struck a shuttle during flight the results could be disastrous, as the shuttle contains sensitive vital electronics and flammable propellant. The rocket's pyrotechnic system – the fuel materials that undergo chemical reactions to ignite and thrust the shuttle space-ward – could easily ignite if hit with a powerful electric shock.
"The two original belts are quite distinct within zone.
But the fact is that you can map almost any number of belts,
depending on what kind of particle you're interested in."
The closest call came when the Apollo 12 spacecraft's external radiation sensors detected a minor flare,
but the interior sensors did not indicate that any appreciable amount of this radiation penetrated the spacecraft hull.
1978
Apr 29/0445 Apr 30/2000 (peak proton flux)
1,000 (PFU >10MeV)
Apr 28/1306 (Flare occurred)
X5/4B
1985
Apr 24/1515 Apr 24/2330
160
Apr 24/1400
X5/2B
1990
May 21/2355 May 22/0750
410
May 21/2219
X5/2B
2000
Jul 14/1045 Jul 15/1230
24,000 (wow!)
Jul 14/1024
X5/3B
particle intensities can rise above this limit to a peak when the shock itselfpasses over the observer creating a ‘delayed’ radiation hazard, even for protons with energies up to ~1 GeV. The streaming limit makes us blind to the intensities at the oncoming shock...
As we consider long-duration missions to the moon or Mars or on the International Space Station(ISS) at high latitude, the risk from rare large events increases. Protons of ~30 MeV penetrate spacesuits and spacecraft walls, those of 130 MeV require 20 g cm-2 of shielding. Events, like that of 1972 August 4, would havebeen fatal to poorly shielded astronauts and large events of 1989 September and October produced significant doses, as did the event of 2000 July 14.
... Soft radiation, with E ~40 MeV, begins to penetrate spacecraft walls, while hard radiation, with E >130MeV, can penetrates 5 cm of Al and becomes extremely difficult to shield. Behind 10 g cm-2 of material astro-nauts would receive a dose ~4 rem hr-1 at intensities in the 1989 September event, accumulating their annual doselimit, currently 50 rem...
(I must say, when I first discovered this document, my jaw was on the floor, you must of saw this coming right Phage)
At 20% comes out to at least 2 of those flares would release
energetic proton fluxes... but wait...
We know all those flares have fluxes
www.fin.ucar.edu...
(1) We found that about only 3.5% (1.9% for M-class and 21.3% for X-class) of the flares are associated with the proton events. (2) It is also found that this fraction strongly depends on longitude; for example, the fraction for 30°W < L ≤ 90°W is about three times larger than that for 30°E < L ≤90°E.
Originally posted by FoosM
..Forum member Phage proves once and for all, that it is not true.
Major Solar Flares did occur during Apollo.
Originally posted by FoosM
Feel free to PROVE that these flares did not emit any energetic proton flux.
Go find that data in your NASA / NOAA websites and show it to us.
Or better, from independent third parties.
Until someone does so, every single one of those flares caused an interstellar SPE.
Originally posted by CHRLZ
Originally posted by CHRLZ
Originally posted by Exuberant1
Your arguments are quite sound and would be better if they did not contain insults. It is a pity you could not go back and edit them all out, as this thread would be an excellent research resource without them. Alas.
Exuberant won't see this (the 'champion of debate' has me blocked..) but I would URGE the other members here to make exuberant responsible for his words. He should be asked to back up his very clear inference that many or all of Pinke's arguments contain insults.
If he cannot back that up, he should have the cojones to admit he was wrong, and APOLOGISE.
Well, Exuberant has been back to ATS since this, and has posted not once... but ten times on other threads.
Yet he HASN'T returned here. Hoping everyone will forget? Hasn't got the intestinal fortitude to admit error and to apologise?
Make your own judgment, dear reader. Is he a 'champion of debate'?