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tatyana61 [14]
3 years ago
8

Explanation of the physics involved i the northern lights(aurora borealis) why can't it occur in mire southerns latitudes?

Physics
1 answer:
PSYCHO15rus [73]3 years ago
5 0

Answer:

The northern lights come from the interaction of electrically charged particles given off by the Sun surface during solar storms and the Earth's magnetic field which is pointed in the northern to southern poles of the Earth. Therefore, the charged particles that travel through millions of miles from the Sun to the Earth accelerate towards the magnetic poles and appear as the northern (and southern) lights

Boreal is an adjective word for the north or northern regions. In the southern latitudes, in the southern hemisphere, the phenomenon is called aurora australis (australis is the adjective for 'of the south')

Explanation:

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What does every magnet possess?
snow_lady [41]

All magnets possess a property called polarity--that is, a magnet's power of attraction is strongest at its opposite ends, usually called the north and south poles. The north and south poles attract each other, but north repels north and south repels south. All magnets attract iron.

8 0
3 years ago
Approximately _____ of those who suffer from anorexia nervosa literally starve themselves to death.
Vadim26 [7]
Appproximately 10% of those who suffer from anorexia nervosa literally starve themselves to death.
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Starting from rest, a wheel with constant angular acceleration turns through an angle of 25 rad in a time t. What will its angul
alexandr402 [8]

Answer:

θ = 225 rad

Explanation:

given data

angle = 25 rad

to find out

angular velocity after 3t?

solution

let angular acceleration α in t

θ = ω × t + 0.5 × α × t²        ........................1

here ω  = 0 (initial velocity )

so put this value here

25 = 0 + 0.5 × α × t²             ..........................2

α = 25 ÷ (0.5 t²)

α = 50 ÷ t²                            .........................3

now here we take in 3t

θ = ω × 3t + 0.5 × α × (3t)²

for ω  = 0

θ = 0 + 0.5 × α × 9t²

now put value in eq 2

so

θ = (0.5) ×  (50 ÷ t²) ×  (3t)²

θ = 25 × 9

θ = 225 rad

6 0
3 years ago
When we stretch a spring, which two factors affect how much elastic
sveta [45]
Mass and gravitational field

3 0
2 years ago
A student is trying to decide what to wear. His bedroom is at 20.0°C. His skin temperature is 30.0°C. The area of his exposed sk
Advocard [28]

Answer:

Explanation:

Stefan's Boltzman Law gives the value of radiation from a black body at a particular temperature. The relation is

E = eσ ( T₂⁴ -T₁⁴ )

e is emmisivity , σ is a constant = 5.67 x 10⁻⁸ , E is energy emitted per unit time per unit area

E = .915 x 5.67 x 10⁻⁸ x ( 303⁴ -293⁴ )

= .915 x 5.67 x 10⁻⁸ x ( 84.28 -73.70 ) x 10⁸

= 55 W / m²s

Area A = 1.45 m²

time t = 14.3 min

= 858 s

Total radiation

= 55 x 858 x 1.45 W

= 68425 J

5 0
3 years ago
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