Orders of magnitude (radiation)

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Recognized effects of higher acute radiation doses are described in more detail in the article on radiation poisoning. Although the International System of Units (SI) defines the sievert (Sv) as the unit of radiation dose equivalent, chronic radiation levels and standards are still often given in units of millirems (mrem), where 1 mrem equals 1/1,000 of a rem and 1 rem equals 0.01 Sv. Light radiation sickness begins at about 50–100 rad (0.5–1 gray (Gy), 0.5–1 Sv, 50–100 rem, 50,000–100,000 mrem).

The following table includes some dosages for comparison purposes, using millisieverts (mSv) (one thousandth of a sievert). The concept of radiation hormesis is relevant to this table – radiation hormesis is a hypothesis stating that the effects of a given acute dose may differ from the effects of an equal fractionated dose. Thus 100 mSv is considered twice in the table below – once as received over a 5-year period, and once as an acute dose, received over a short period of time, with differing predicted effects. The table describes doses and their official limits, rather than effects.

Level (mSv) Level in standard form (mSv) Duration Hourly equivalent (μSv/hour) Description
0.001 1×10^−3 Hourly 1 Cosmic ray dose rate on commercial flights varies from 1 to 10 μSv/hour, depending on altitude, position and solar sunspot phase.[1]
0.01 1×10^−2 Daily 0.4 Natural background radiation, including radon[2]
0.06 6×10^−2 Acute - Chest X-ray (AP+Lat)[3]
0.07 7×10^−2 Acute - Transatlantic airplane flight.[1]
0.09 9×10^−2 Acute - Dental X-ray (Panoramic)[3]
0.1 1×10^−1 Annual 0.011 Average USA dose from consumer products[4]
0.15 1.5×10^−1
0.25
0.27 2.7×10^−1 Annual 0.031 Yearly dose from natural cosmic radiation at sea level (0.5 in Denver due to altitude)[4]
0.28 2.8×10^−1 Annual 0.032 USA yearly dose from natural terrestrial radiation (0.16-0.63 depending on soil composition)[4]
0.46
0.48
0.66 6.6×10^−1 Annual 0.075 Average USA dose from human-made sources[2]
0.7 7×10^−1 Acute - Mammogram[3]
1 1×10^0 Annual 0.11 Limit of dose from man-made sources to a member of the public who is not a radiation worker in the US and Canada[2][5]
1.1 1.1×10^0 Annual 0.13 Average USA radiation worker occupational dose in 1980[2]
1.2 1.2×10^0 Acute - Abdominal X-ray[3]
2 2×10^0 Annual 0.23 USA average medical and natural background [2]
Human internal radiation due to radon, varies with radon levels[4]
2 2×10^0 Acute - Head CT[3]
3 3×10^0 Annual 0.34 USA average dose from all natural sources[2]
3.66
4 4×10^0 Duration of the pregnancy 0.6 Canada CNSC maximum occupational dose to a pregnant woman who is a designated Nuclear Energy Worker.[5]
5 5×10^0 Annual 0.57 USA NRC occupational limit for minors (10% of adult limit)
USA NRC limit for visitors[6]
5
6.4 6.4×10^0 Annual 0.73 High Background Radiation Area (HBRA) of Yangjiang, China[7]
7.6
8 8×10^0 Acute - Chest CT[3]
10 1×10^1 Acute - Lower dose level for public calculated from the 1 to 5 rem range for which USA EPA guidelines mandate emergency action when resulting from a nuclear accident[2]
Abdominal CT[3]
14 1.4×10^1 Acute - 18F FDG PET scan,[8] Whole Body
50 5×10^1 Annual 5.7 USA NRC/ Canada CNSC occupational limit for designated Nuclear Energy Workers[5](10 CFR 20)
100 1×10^2 5 years 2.3 Canada CNSC occupational limit over a 5-year dosimetry period for designated Nuclear Energy Workers[5]
100 1×10^2 Acute - USA EPA acute dose level estimated to increase cancer risk 0.8%[2]
120 1.2×10^2 30 years 0.46 Exposure, long duration, Ural mountains, lower limit, lower cancer mortality rate[9]
150
170 1.7×10^2 Acute Average dose for 187,000 Chernobyl recovery operation workers in 1986[10][11]
175
250 2.5×10^2 2 hours 125,000 (125 mSv/hour) Whole body dose exclusion zone criteria for US nuclear reactor siting[12] (converted from 25 rem)
250 2.5×10^2 Acute - USA EPA voluntary maximum dose for emergency non-life-saving work[2]
260 2.6×10^2 Annual 30 Calculated from 260 mGy per year peak natural background dose in Ramsar[13]
400-900 4–9×10^2 Annual 46-103 Unshielded in interplanetary space.[14]
500 5×10^2 Annual 57 USA NRC occupational whole skin, limb skin, or single organ exposure limit
500 5×10^2 Acute - Canada CNSC occupational limit for designated Nuclear Energy Workers carrying out urgent and necessary work during an emergency.[5]
Low-level radiation sickness due to short-term exposure[15]
750 7.5×10^2 Acute - USA EPA voluntary maximum dose for emergency life-saving work[2]
1,000 10×10^2 Hourly 1,000,000 Level reported during Fukushima I nuclear accidents, in immediate vicinity of reactor[16]
3,000 3×10^3 Acute - Thyroid dose (due to iodine absorption) exclusion zone criteria for US nuclear reactor siting[12] (converted from 300 rem)
4,800 4.8×10^3 Acute - -1">50 (actually LD50/60) in humans from radiation poisoning with medical treatment estimated from 480 to 540 rem.[17]
5,000 5×10^3 Acute - Calculated from the estimated 510 rem dose fatally received by Harry Daghlian on August 21, 1945, at Los Alamos and lower estimate for fatality of Russian specialist on April 5, 1968, at Chelyabinsk-70.[18]
5,000 5×10^3 5,000 - 10,000 mSv. Most commercial electronics can survive this radiation level.[19]
16,000 1.6×10^4 Acute Highest estimated dose to Chernobyl emergency worker diagnosed with acute radiation syndrome[11]
20,000 2×10^4 Acute 2,114,536 Interplanetary exposure to solar particle event (SPE) of October 1989.[20][21]
21,000 2.1×10^4 Acute - Calculated from the estimated 2,100 rem dose fatally received by Louis Slotin on May 21, 1946, at Los Alamos and lower estimate for fatality of Russian specialist on April 5, 1968 Chelyabinsk-70.[18]
48,500 4.85×10^4 Acute - Roughly calculated from the estimated 4,500 + 350 rad dose for fatality of Russian experimenter on June 17, 1997, at Sarov.[18]
60,000 6×10^4 Acute - Roughly calculated from the estimated 6,000 rem doses for several Russian fatalities from 1958 onwards, such as on May 26, 1971, at the Kurchatov Institute. Lower estimate for fatality of Cecil Kelley at Los Alamos on December 30, 1958.[18]
100,000 1×10^5 Acute - Roughly calculated from the estimated 10,000 rad dose for fatality at the United Nuclear Fuels Recovery Plant on July 24, 1964.[18]
30,000,000 3×10^7 3,600,000 Radiation tolerated by Thermococcus gammatolerans, a microbe extremely resistant to radiation.[22]
10,000,000,000 1×10^10 The most radiation-hardened electronics can survive this radiation level.[23]
70,000,000,000 7×10^10 Hourly 70,000,000,000,000 Estimated dose rate for the inner wall in ITER (2 kGy/s with an approximate weighting factor of 10)[24]
Comparison of Radiation Doses - includes the amount detected on the trip from Earth to Mars by the RAD on the MSL (2011 - 2013).[25][26][27][28]

See also

External links

References

  1. "Annex B: Exposures from natural radiation sources". UNSCEAR 2000 Report: Sources and Effects of Ionizing Radiation. 1 Sources. p. 88, Figure 3. http://www.unscear.org/docs/reports/annexb.pdf. 
  2. 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 2.8 Oak Ridge National Laboratory (http://www.ornl.gov/sci/env_rpt/aser95/tb-a-2.pdf )
  3. 3.0 3.1 3.2 3.3 3.4 3.5 3.6 Health Physics Society (http://www.hps.org/documents/meddiagimaging.pdf)
  4. 4.0 4.1 4.2 4.3 Oak Ridge National Laboratory (http://www.ornl.gov/sci/env_rpt/aser95/appa.htm )
  5. 5.0 5.1 5.2 5.3 5.4 Radiation Protection Regulations, Canada
  6. "Annex B: Exposures from natural radiation sources". UNSCEAR 2000 Report: Sources and Effects of Ionizing Radiation. 1 Sources. http://www.unscear.org/docs/reports/annexb.pdf. "Orvieto town, Italy" 
  7. "[Cancer mortality in high background radiation area of Yangjiang, China, 1979–1995]" (in zh). Zhonghua Yi Xue Za Zhi 79 (7): 487–92. July 1999. PMID 11715418. 
  8. "Radiation Exposure from Medical Exams and Procedures". http://hps.org/documents/Medical_Exposures_Fact_Sheet.pdf. 
  9. "Pollycove 2000 Symposium on Medical Benenfits of LDR". http://cnts.wpi.edu/RSH/Docs/Pollycove2000_Symp_on_Med_Ben.htm. 
  10. UNSCEAR 2000 Report, Annex J, Exposures and effects of the Chernobyl Accident. United Nations Scientific Committee on the Effects of Atomic Radiation. 2000. p. 526. http://www.unscear.org/docs/reports/2000/Volume%20II_Effects/AnnexJ_pages%20451-566.pdf. 
  11. 11.0 11.1 "Chernobyl: Assessment of Radiological and Health Impact. Chapter IV Dose estimates". OECD Nuclear Energy Agency. 2002. https://www.oecd-nea.org/rp/chernobyl/c04.html. 
  12. 12.0 12.1 10 CFR Part 100.11 Section 1
  13. Dissanayake C (May 2005). "Of Stones and Health: Medical Geology in Sri Lanka". Science 309 (5736): 883–5. doi:10.1126/science.1115174. PMID 16081722. "high as 260 mGy/year". 
  14. R.A. Mewaldt (2005-08-03). "The Cosmic Ray Radiation Dose in Interplanetary Space – Present Day and Worst-Case Evaluations". 29th International Cosmic Ray Conference Pune (2005) 00, 101-104. p. 103. http://www.srl.caltech.edu/ACE/ASC/DATA/bibliography/ICRC2005/usa-mewaldt-RA-abs1-sh35-oral.pdf. 
  15. Centers for Disease Control and Prevention (https://emergency.cdc.gov/radiation/ars.asp)
  16. "Japan's Chernobyl". Spiegel. 2011-03-14. http://www.spiegel.de/international/world/0,1518,750773,00.html. 
  17. Biological Effects of Ionizing Radiation
  18. 18.0 18.1 18.2 18.3 18.4 "A Review of Criticality Accidents". Los Alamos National Laboratory. May 2000. pp. 16, 33, 74, 75, 87, 88, 89. http://www.orau.org/ptp/Library/accidents/la-13638.pdf. 
  19. ieee.org - Radiation Hardening 101: How To Protect Nuclear Reactor Electronics
  20. "Mars Surface Radiation Exposure for Solar Maximum Conditions and 1989 Solar Proton Events". February 1993. p. 9. https://www.solarstorms.org/NASATech3300.pdf. 
  21. Torsti, J.; Anttila, A.; Vainio, R. l Kocharov (1995-08-28). "Successive Solar Energetic Particle Events in the October 1989". International Cosmic Ray Conference 4: 140. 2016-02-17. Bibcode1995ICRC....4..139T. 
  22. Jolivet, Edmond; L'Haridon, Stéphane; Corre, Erwan; Forterre, Patrick; Prieur, DanielYR 2003 (2003). "Thermococcus gammatolerans sp. nov., a hyperthermophilic archaeon from a deep-sea hydrothermal vent that resists ionizing radiation". International Journal of Systematic and Evolutionary Microbiology 53 (3): 847–851. doi:10.1099/ijs.0.02503-0. ISSN 1466-5034. PMID 12807211. https://www.microbiologyresearch.org/content/journal/ijsem/10.1099/ijs.0.02503-0. 
  23. "RD53 investigation of CMOS radiation hardness up to 1Grad". https://indico.cern.ch/event/302139/session/13/contribution/176/material/slides/0.pdf. 
  24. Henri Weisen: ITER Diagnostics, page 13. Accessed August 28, 2017
  25. Kerr, Richard (31 May 2013). "Radiation Will Make Astronauts' Trip to Mars Even Riskier". Science 340 (6136): 1031. doi:10.1126/science.340.6136.1031. PMID 23723213. Bibcode2013Sci...340.1031K. https://www.science.org/doi/abs/10.1126/science.340.6136.1031. Retrieved 31 May 2013. 
  26. Zeitlin, C. (31 May 2013). "Measurements of Energetic Particle Radiation in Transit to Mars on the Mars Science Laboratory". Science 340 (6136): 1080–1084. doi:10.1126/science.1235989. PMID 23723233. Bibcode2013Sci...340.1080Z. https://www.science.org/doi/abs/10.1126/science.1235989. Retrieved 31 May 2013. 
  27. Chang, Kenneth (30 May 2013). "Data Point to Radiation Risk for Travelers to Mars". New York Times. https://www.nytimes.com/2013/05/31/science/space/data-show-higher-cancer-risk-for-mars-astronauts.html. 
  28. Gelling, Cristy (June 29, 2013). "Mars trip would deliver big radiation dose; Curiosity instrument confirms expectation of major exposures". Science News 183 (13): 8. doi:10.1002/scin.5591831304. http://www.sciencenews.org/view/generic/id/350728/description/Mars_trip_would_deliver_big_radiation_dose. Retrieved July 8, 2013.