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пи Pӛ

l(f)rg:2017-05-26݋f

ב(yng)ԓЧӛ Pӛ?СVĂɲ֪и ӛPӛļ!gӭx!

һfи ԇһsectionһԒ̓ɂvЌԒֵLͨ2-3nvtҪLһЩЩ_(d)5-6҂֪и 헟oՓǂ俼߀yȶǷdzģ σ(ni)漰VҌI(y)ԘO(qing)@ҪHҪ֪֪ҪƼˇvʷ˽⡣

(dng)ȻҪϵ֪RȫĻDzܵ҂ľǏ ȡP(gun)֪R@rӛPӛ׃҂Qи ԇP(gun)I@Ҳи ώڽ̌W(xu)Џ(qing){(dio)ӛPӛҪԵԭoՓ뱣15ֵĿ߀_30ֵĿֻҪҪ(zhn)_İи µ挍xPӛɲ

ӛPӛT̎Ԏ㼯ע߀Լӏ(qing)̕rӛԎ ϵļ(x)(ji)λcǷذl(f)F(xin)Լ(x)һmȻ µĕr^βӛ˺ܶPӛsΨ]ӛc?}rl(f)F(xin)ԼȻԼĹPӛ?ֻһӛPӛ© ܶ༚(x)(ji)(do)ºƒ(ni) Լ߉݋Ҳy?

һ ԒӛP(gun)I~

vӛи Pӛķrώһһ_ʼ͕V㣺ӛP(gun)I~ļ^P(gun)I~һָһЩҪČ~f~~~ͷ~Ȼ@Ҫעǣ҂Ҫ @Ȼͬ׽סĂ~@ҪϢ@ĿP(gun)I~}rؑ

eӣČԒW(xu)ώԃӌώٵfһBҊ@ͺܿܳx}@r҂ҪڹPӛwF(xin)еҊô҂ԓӛЩ~?

Student: Do you have any advice on how I should cover the story?

Advisor: Well, Max will want to talk to you but I am sure he will tell you to find out things like why the physics department's worried about enrollment?Has the number of students been getting smaller in recent years? By how much? What kinds of plans are they considering to address this problem?

τfķ挦ԒЮֵľwҊҪӛ~R(yng)ԓ@ӣworried?No. stu?how?plan?

ӛ䛾߉݋P(gun)ϵ~׳c

߉݋BһƪµĽ}j(lu)ÿһƪи ¶(yn)֔(jn)?sh)ŒӴκ߉݋P(gun)ϵ֮gҊ߉݋P(gun)ϵD(zhun)ۡ혳e߉݋ͨ^߉݋~߉݋ZwF(xin)ġһF(xin)߉݋~ͺܸܿc

 ߉݋~Ѹӛ܉ʹƒ(ni)P(gun)ϵһĿȻ

õѸӛ䛾g߉݋P(gun)ϵķͨ^N̖磺

Ѵңõ߉݋R܉ճҊ߉݋~ԼZ@ӟoՓڜyԇx Zֵĕrһ(yu)܉ƽr Ӗ(xn)ע⿂Y(ji)@Щ߉݋~ͶZ÷\(yn)ԼĿZ֣͌һ܉M(jn)߷֙n

 ĄemY(ji)cӛҪϢ

Ŵ(sh)ͬW(xu)@ӵw(dng)҂ µ^У һ̫Ć~ӕr˼Sͣ@~ϣͬr© ˽ϢȻ^񃺁Űl(f)F(xin)ѽ(jng)֪făȥ

䌍и ԇ(dng)F(xin)ҪϢƧĆ~ĕrvԒ߽^󲿷r¶ԽǷ(f)@Ϣ~҂Ҫľ ~ĕrסě_Ӳ^Ƥ  ~Ľ֮ڹPӛӛҪϢ҂Ҫעǣи з(f)F(xin)ጵϢһҪϢOпǿcҲҪ҂cӛPӛĵط

ώoeһֱܷĶfˎׂҪϢ?

Ok, a lot of people think of earth’s orbit around the sun as being perfectly circular, as smooth and as regular as, say, the way that hands move on a well-made watch, but it just doesn’t work that way. You are probably aware that the earth’s orbit around the sun, it is not shaped like a perfect circle. It is more of an oval, it is elliptical. But the shape of this orbit isn’t consistent; it varies over time, over a period of about a thousand years. Sometimes it is a little more circular, sometimes it is more elliptical. And when earth’s orbit is more elliptical, earth is actually closer to the sun during part of the year. Which makes earth, and in particular, the northern hemisphere, warmer. And why is that important? Well, because most of the planet’s glaciers are in the northern hemisphere, and if it gets too warm, then glaciers will stop forming. And we’ve already talked about how that affects earth’s overall temperature.

䌍e@@ôL䌍ֻ_(d)ҪϢҲfw{ֻcIJֶnjcĽ

һϢ@̫ꖵ܉ǙEAεԭ5Ԓ(f)@ϢmȻF(xin)ƧĆ~oval}¿ һ^Ҋelliptical£

Ok, a lot of people think of earth’s orbit around the sun as being perfectly circular, as smooth and as regular as, say, the way that hands move on a well-made watch, but it just doesn’t work that way. You are probably aware that the earth’s orbit around the sun, it is not shaped like a perfect circle. It is more of an oval, it is elliptical.

ڶϢ@܉Π׃@5Ԓ(f)ጣгF(xin)һ΢ЩyȵĆ~consistentҷֹЩJ(rn)R@~}ֿĵĽo@F(xin)Еr@܉ΠAcЕrEAcEAcĕr򣬵ӽ̫@fľ҂ЌW(xu)֪RеĽc@

But the shape of this orbit isn’t consistent; it varies over time, over a period of about a thousand years. Sometimes it is a little more circular, sometimes it is more elliptical. And when earth’s orbit is more elliptical, earth is actually closer to the sun during part of the year.

ϢΠ׃Ӱ푵ϱγfԒһ5Ԓ@Ϣ㲻֪@Ҫc߀˷㡣

Which makes earth, and in particular, the northern hemisphere, warmer. And why is that important? Well, because most of the planet’s glaciers are in the northern hemisphere, and if it gets too warm, then glaciers will stop forming. And we’ve already talked about how that affects earth’s overall temperature.

mȻ @ô~R;ӣ䌍ĹPӛҪӛֻ@ҪϢɴ˿֪ETSһԻĵĽM(dng) ϢĕrҪ¸҈ԛQ^m(x) ˼SҪͬrfԒ^ܳF(xin)Լ˼Sӡ

˽и v}·Д(sh)Ųy

и vֵ·к܏(qing)Ҏ(gu)Եһf֞6E

һϹ(ji)n(ni)

ڶ~(@(ji)n})

B@~(һNF(xin)󣬻vʷ¼)

IJͨ^eķʽ߽B̵ķʽU}ľw(ni)

岽v^дW(xu)ᆖώԼᆖ֮o (ÿᆖ̎ܿǿc)

}M(jn)пY(ji)A(ᵽv}^ȥδa(chn)Ӱ푻h(yun)x)

(dng)˽и vֵ·ҪƽrĹPӛӖ(xn)^Rذ Ϣw{M(jn)@·@܉õذ½Y(ji)(gu)܉_(d)?jng)] ÿһϢҲ}ľ

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