Sievert to Microsievert

At 1 Sv: nausea, vomiting, and fatigue within hours; blood cell counts drop but most people survive with supportive care. At 3 Sv: severe bone marrow damage, bleeding, infection risk, hair loss — survival is possible (~50% with intensive treatment) but uncertain. At 6 Sv: near-total bone marrow destruction plus gastrointestinal damage; even with aggressive treatment including bone marrow transplant, survival is unlikely. Above 10 Sv the gut lining disintegrates and death occurs within days regardless of treatment. These thresholds apply to whole-body, acute exposure — the same total dose spread over months causes far less harm.

Alpha particles are massive (two protons + two neutrons) and highly charged, so they dump all their energy in a tiny volume of tissue — a few cell diameters. That concentrated damage creates complex, hard-to-repair DNA double-strand breaks. Gamma photons spread their energy thinly across a larger volume, causing simpler damage that cells repair more easily. The radiation weighting factor (w_R = 20 for alphas, 1 for gammas) converts absorbed dose in gray to equivalent dose in sieverts, capturing this biological difference. It is a simplification — the real damage depends on many factors — but it works well enough for radiation protection.

ISS crew receive about 0.5–1 mSv per day — roughly 150–200 mSv during a six-month mission — primarily from galactic cosmic rays and occasional solar particle events. NASA limits career dose based on age and sex (historically 1–4 Sv lifetime, recently standardized to 600 mSv), monitored via personal dosimeters and area monitors. During solar storms, crew shelter in the most heavily shielded module (usually near the water tanks). A Mars mission would deliver roughly 1 Sv total, pushing against career limits and making radiation the single biggest health obstacle to deep space travel.

This is one of the most debated questions in radiation science. The "linear no-threshold" (LNT) model, used by most regulators, assumes every additional dose carries some cancer risk proportional to the dose — so there is no perfectly safe level. Critics point out that below about 100 mSv, the added risk is too small to detect statistically against the high natural cancer rate. Some researchers argue low doses may even stimulate repair mechanisms (hormesis). Current regulatory policy uses LNT as a conservative precaution, not because there is proof of harm at very low doses.

Rolf Sievert spent decades in the early-to-mid 1900s building dosimetry instruments and gathering data on how radiation damages living tissue. His work showed that the physical dose (energy deposited) and the biological effect (tissue damage) are not the same thing — you need weighting factors for radiation type and tissue sensitivity. The ICRP formalised this into the concepts of equivalent dose and effective dose, and the 1979 CGPM named the unit after Sievert. One sievert of any radiation type, to any tissue, is supposed to carry the same overall cancer risk — a bold simplification that works reasonably well in practice.

A New York-to-London flight delivers roughly 50–80 µSv of cosmic radiation, depending on solar activity and the specific flight path over the pole. That is equivalent to about 3–4 chest X-rays. Pilots and cabin crew who fly long-haul routes accumulate 2–5 mSv per year — enough that airlines in the EU are legally required to monitor their doses. Passengers on a once-a-year vacation flight have nothing to worry about; frequent business travellers crossing the Atlantic weekly might accumulate a few extra millisieverts annually, still well within safe limits.

A dental bitewing exposes a few square centimeters of jaw to a brief, low-energy X-ray pulse — about 5 µSv. A chest CT scans the entire thorax in a spiral, delivering radiation from every angle to build a 3D image — roughly 7,000 µSv. The dose difference (about 1,400×) comes from three factors: the area exposed, the beam energy, and the duration. Dental X-rays use narrow, collimated beams at 60–70 kVp for milliseconds; CT scanners use wide fans at 120 kVp for several seconds of continuous rotation.

No. Radiation is completely imperceptible to human senses at any dose below the threshold for acute radiation syndrome (roughly 250,000 µSv as a sudden whole-body exposure). You cannot feel a chest X-ray, a CT scan, or even the elevated cosmic radiation at cruising altitude. The only "sensation" from radiation occurs at extremely high doses — a metallic taste reported by some Chernobyl liquidators, which was likely caused by ozone and nitrogen oxides generated by intense gamma fields ionising the air, not by direct neural stimulation.

A dosimeter records the cumulative equivalent dose to the wearer, typically in µSv or mSv. Film badges (now largely replaced), thermoluminescent dosimeters (TLDs), and optically stimulated luminescence (OSL) badges are worn monthly then read by a lab. Electronic personal dosimeters (EPDs) give real-time µSv/hr readings with audible alarms. Nuclear workers, radiologists, interventional cardiologists, industrial radiographers, and airline crew in some countries are all required to wear them. The legal dose limit for most workers is 20 mSv/year.

No — phones and Wi-Fi emit non-ionising radio-frequency radiation, which does not cause the kind of DNA damage that ionising radiation (X-rays, gamma rays, alpha particles) causes. Microsieverts apply exclusively to ionising radiation. Radio waves are measured in watts per kilogram (specific absorption rate, or SAR) for phones, and microwatts per square centimeter for environmental RF. Comparing a phone signal to a chest X-ray in microsieverts is like comparing the temperature of a warm bath to the speed of a car — they are fundamentally different physical quantities.