2014иԇ(jng)(yn)и (tng)
r(sh)g2014-12-18 17:14:00 (li)Դ|ھ(xin) I [wС ]һ(li)f(shu)и (tng)ԇһ(g)sectionһ(g)(du)Ԓ(hu)̓ɂ(g)vЌ(du)Ԓ(hu)ֵL(zhng)ͨ2-3nvtҪL(zhng)һЩЩ_(d)5-6҂֪֣и (tng)(xing)o(w)Փǂ俼߀yȶǷdzģ?yn)?tng)σ(ni)漰VҌ(zhun)I(y)ԘO(qing)@ҪHҪ֪֪Ҫ(du)Ƽˇvʷ˽
(dng)ȻҪϵ֪R(sh)ȫĻDzܵ҂ľǏ (tng)ȡP(gun)֪R(sh)@r(sh)ӛPӛ׃҂Qи (tng)ԇP(gun)I@Ҳи (tng)ώڽ̌W(xu)Џ(qing){(dio)ӛPӛҪԵԭo(w)Փ뱣15ֵĿ߀_30ֵĿֻҪҪ(zhn)_İи (tng)µ挍(sh)xPӛɲ
ӛPӛT̎Ԏ㼯ע߀Լӏ(qing)̕r(sh)ӛԎ (tng)ϵļ(x)(ji)λc(din)ǣǷذl(f)F(xin)Լ(x)һ(g)mȻ (tng)µĕr(sh)^βӛ˺ܶPӛsΨ(d)](mi)ӛc(din)}r(sh)l(f)F(xin)ԼȻԼĹPӛֻһӛPӛ© (tng)ܶ༚(x)(ji)(do)º(ni) (tng)Լ߉Ҳy
ôב(yng)ԓЧӛ (tng)Pӛ|ھ(xin)иώ(li)VĂ(g)ɲ֪и (tng)ӛPӛļɣ
һ (tng)Ԓ(hu)ӛP(gun)I~
vӛи (tng)Pӛķr(sh)ώһһ_(ki)ʼ͕(hu)V㣺ӛP(gun)I~ǻļ^P(gun)I~һָһЩҪČ(sh)~f(shu)~(dng)~~ͷ~Ȼ@Ҫעǣ҂Ҫ (tng)@(g)ӣȻͬסĂ(g)~@(g)ҪϢ@(g)ĿP(gun)I~(li)}r(sh)ؑ(g)ӡ
e(g)Č(du)Ԓ(hu)УW(xu)ώԃ(xn)(wn)ӌ(xi)(bo)ώٵf(shu)һBҊ(jin)@ͺܿܳx}@r(sh)҂ҪڹPӛwF(xin)еҊ(jin)ô҂?c)ӛЩ~
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 enrollmentHas the number of students been getting smaller in recent years? By how much? What kinds of plans are they considering to address this problem?
τf(shu)ķ挦(du)Ԓ(hu)Ю(hu)(xin)ֵľwҊ(jin)Ҫӛ(li)~R(yng)ԓ@ӣworriedNo. stuhowplan
ӛ䛾߉P(gun)ϵ~׳c(din)
߉BһƪµĽ}j(lu)ÿһƪи (tng)¶(yn)֔(jn)?sh)Ӵκ߉P(gun)ϵ֮gҊ(jin)߉P(gun)ϵD(zhun)ۡ(du)ȡ혳e߉ͨ^(gu)߉~߉Z(y)(li)wF(xin)һF(xin)߉~ͺܸܿc(din) (tng)߉~Ѹӛ(li)܉ʹ(ni)P(gun)ϵһĿȻ
ӛ̖(ho) | ߉~ |
different, unlike, contradict, rather than | |
<> | belong to, be part of |
due to, because, reason | |
but, however, yet, in fact, actually, while |
õѸӛ䛾g߉P(gun)ϵķͨ^(gu)N̖(ho)磺
ӛ̖(ho) | ߉~ |
different, unlike, contradict, rather than | |
<> | belong to, be part of |
due to, because, reason | |
but, however, yet, in fact, actually, while |
|ھ(xin)иԇώѴõ߉R(sh)܉ճҊ(jin)߉~ԼZ(y)@ӟo(w)Փڜy(c)ԇx (tng)Z(y)IJֵĕr(sh)һ(g)(yu)(sh)܉ƽr(sh) (tng)Ӗ(xn)ע⿂Y(ji)@Щ߉~ͶZ(y)÷\(yn)ԼĿZ(y)͌(xi)һ܉M(jn)߷֙n
(tng)ĄemY(ji)c(din)ӛҪϢ
Ŵ(sh)ͬW(xu)@ӵw(hu)(dng)҂?c)?tng)µ^(gu) (tng)һ(g)̫Ć~ӕr(sh)(hu)˼Sͣ@(g)~ͬr(sh)© (tng)˽(li)ϢȻ^(gu)(li)Űl(f)F(xin)ѽ(jng)֪f(shu)ăȥ
䌍(sh)и (tng)ԇУ(dng)F(xin)ҪϢƧĆ~ĕr(sh)vԒ(hu)߽^r¶(hu)Խ?zhun)Ƿ?f)@(g)Ϣ~҂Ҫľ (tng)~ĕr(sh)סě_(dng)Ӳ^Ƥ (tng) (tng)~Ľ֮ڹPӛӛҪϢң҂Ҫעи (tng)з(f)F(xin)ጵϢһҪϢOпǿc(din)ҲҪ҂c(din)ӛPӛĵط
|ھ(xin)иԇώoeһ(g)(li)ֱܷĶf(shu)ˎׂ(g)ҪϢ
Ok, a lot of people think of earths 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 doesnt work that way. You are probably aware that the earths 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 isnt 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 earths 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 planets glaciers are in the northern hemisphere, and if it gets too warm, then glaciers will stop forming. And weve already talked about how that affects earths overall temperature.
䌍(sh)e@(g)@ôL(zhng)䌍(sh)ֻ_(d)(g)ҪϢҲf(shu)w{(li)ֻ(g)c(din)IJֶnj(du)c(din)Ľጡ
һ(g)Ϣ@̫(yng)܉ǙEAεԭ5Ԓ(hu)(li)(f)@(g)ϢmȻF(xin)(du)ƧĆ~oval}¿ (tng)һ(g)^Ҋ(jin)elliptical(li)£
Ok, a lot of people think of earths 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 doesnt work that way. You are probably aware that the earths orbit around the sun, it is not shaped like a perfect circle. It is more of an oval, it is elliptical.
ڶ(g)Ϣ@(g)܉Π(hu)׃@5Ԓ(hu)(li)(f)?zhun)гF(xin)һ(g)ЩyȵĆ~consistentҷֹЩJ(rn)R(sh)@(g)~}ֿĵĽo@(g)F(xin)Еr(sh)@(g)܉ΠAc(din)Еr(sh)EAc(din)EAc(din)ĕr(sh)ӽ̫(yng)@f(shu)ľ҂ЌW(xu)֪R(sh)еĽc(din)@(g)
But the shape of this orbit isnt 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 earths orbit is more elliptical, earth is actually closer to the sun during part of the year.
(g)ϢΠ׃(hu)Ӱ푵ϱγɡf(shu)Ԓ(hu)5Ԓ(hu)(li)@(g)Ϣ㲻֪@Ҫc(din)߀˷(wn)
Which makes earth, and in particular, the northern hemisphere, warmer. And why is that important? Well, because most of the planets glaciers are in the northern hemisphere, and if it gets too warm, then glaciers will stop forming. And weve already talked about how that affects earths overall temperature.
mȻ (tng)@ô~R;ӣ䌍(sh)ĹPӛҪӛֻ@(g)ҪϢɴ˿֪ETSһ(g)ԻĵĽM(dng) (tng)Ϣĕr(sh)Ҫ¸҈(jin)Q^m(x) (tng)˼SҪͬr(sh)f(shu)Ԓ(hu)ߣ^ܳF(xin)Լ˼S
ġ˽и (tng)v}·Д(sh)Ųy
и (tng)vֵ·к(qing)Ҏ(gu)Եһ(li)f(shu)֞6(g)E
һϹ(ji)n(ni)
ڶ(zhun)~@(ji)n}
B@(g)(zhun)~һNF(xin)vʷ¼
IJͨ^(gu)e(li)ķʽ߽B̵ķʽ(li)U}ľw(ni)
岽(g)v^(gu)дW(xu)ᆖ(wn)ώԼᆖ(wn)֮o ÿ(g)ᆖ(wn)̎ܿǿc(din)
(du)}M(jn)пY(ji)A(hu)ᵽv}(du)^(gu)ȥδ(li)a(chn)Ӱ푻h(yun)xȣ
(dng)˽и (tng)vֵ·Ҫƽr(sh)ĹPӛӖ(xn)^(gu)R(sh)ذ (tng)Ϣw{M(jn)@(g)·@܉õذ½Y(ji)(gu)܉_(d)?jng)] (tng)ÿһ(g)ϢҲ(du)}ľ硣
Ո(qng)ӛסڂ俼и (tng)^(gu)Pӛľ(x)ͨ (tng)߷ֻM(mn)ֱؽ(jng)Ęϣ܉м(x)w(hu)f(shu)ķN\(yn)õ(x)ףÿһ(g)ȡÝM(mn)ijɿ(j)Ҽ