太阳（）建立了提高销售人员知识水平和 能力的知识管理培训系统，并取名为SunTAN系统，这是一种交互

太阳微系统公司是美国计算机软硬件生产及服务的著名公司之一，其90%的销售额来自

新产品。由于产品系列不断增加，产品生命周期越来越短，因此必须大力加强公司销售能力，

然而传统的集中式课堂培训方式难以满足需要，为此SUN公司利用其强大的公司内部网

SunWE吧(具有1000多台内部Web服务器和25万多网页)建立了提高销售人员知识水平和

能力的知识管理培训系统，并取名为SunTAN系统，这是一种交互作用、基于网络的课程管理

和销售支持系统，通过该系统对分布各地的公司销售人员实施远程教学和信息服务，SunTAN

系统还扮演了即时知识支持系统的角色，系统内的产品目录和技术信息使得销售人员在接听

客户电话咨询时能够快速准确地获取相关信息，满足客户的需要，并增进了与客户的良好关

系。

SunTAN系统的建立和运行，既大大提高了企业销售人员的知识水平和工作效率，又降

低了企业培训成本。据统计，该公司仅每年节省销售人员回总部培训的差旅费就多达7500万

美元。太阳微系统公司的知识培训体系应该是美国企业培训体系的一个缩影。美国企业一直

致力于办企业大学和利用先进的因特网开展网络教学培训。通过因特网实行远程教学和信息

服务，改变了传统集中、被动培训的模式。员工可以随时随地地根据个人需要上网进行学习和

信息利用。既降低了培训成本又提高培训效果。此类培训体系的建立并不需要投人大量的财

力和物力。

案例分析:太阳微系统公司主要从哪些方面开展知识管理，其成效如何?有哪些方面值得

我们借鉴?

It's not surprising that sunspots (太阳黑子) were observed by ancient astronomers (天文学家). The largest sunspots on the sun can be seen without a telescope. It was not until the invention of the telescope (望远镜) in the early 17th century, however, that systematic studies of sunspots could be undertaken. The great astronomer Galileo was among the first to make telescopic observations of sunspots.

Sunspots are regions of extremely strong magnetic fields (磁场) found on the sun's surface. A sunspot has a dark Central core known as the umbra. The umbra is surrounded by a dark ring called the penumbra, where the magnetic field spreads outward. SunSpots appear dark because they are giving off less radiation. They are cooler than the rest of the sun's surface.

Sunspots are frequently observed in pairs or in paired groups. The members of a spot pair are identified as the leading spot and the following spot. They are identified by their position in the pair in terms of the direction in which the sun rotates (旋转).

The number of sunspots at any one time varies. A large spot group may consist of as many as 10 groups and 300 spots across the sun. The number of spots changes in a fairly regular pattern called the sunspot cycle. The largest number occurs about every 11 years. At sunspot minimum, there are at most just a few small spots.

The average lifetime of an individual spot group is roughly one solar rotation, which is about 25 days. The most persistent large spots,' however, can survive for two to three months.

Careful observations and systematic studies of sunspots

A．were made by ancient astronomers.

B．started in the early 17th century.

C．were made by Galileo only.

D．could be made without a telescope.

It's not surprising that sunspots (太阳黑子) were observed by ancient astronomers (天文学家). The largest sunspots on the sun can be seen without a telescope. It was not until the invention of the telescope (望远镜) in the early 17th century, however, that systematic studies of sunspots could be undertaken. The great astronomer Galileo was among the first to make telescopic observations of sunspots.

Sunspots are regions of extremely strong magnetic fields (磁场) found on the sun's surface. A sunspot has a dark central core known as the umbra. The umbra is surrounded by a dark ring called the penumbra, where the magnetic field, spreads outward. Sunspots appear dark because they are giving off less radiation. They are cooler than the rest of the sun's surface.

Sunspots are frequently observed in pairs or in paired groups. The members of a spot pair are identified as the leading spot and the following spot. They are identified by their position in the pair in terms of the direction in which the sun rotates (旋转).

The number of sunspots at any one time varies. A large spot group may consist of as many as 10 groups and 300 spots across the sun. The number of spots changes in a fairly regular pattern called the sunspot cycle. The largest number occurs about every 11 years. At sunspot minimum, there are at most just a few small spots.

The average lifetime of an individual spot group is roughly one solar rotation, which is about 25 days. The most persistent large spots, however, can survive for two to three months.

Careful observations and systematic studies of sunspots

A．were made by ancient astronomers.

B．started in the early 17th century.

C．were made by Galileo only.

D．could be made without a telescope.

It's not surprising that sunspots (太阳黑子) were observed by ancient astronomers (天文学家). The largest sunspots on the sun can be seen without a telescope. It was not until the invention of the telescope (望远镜) in the early 17th century, however, that systematic studies of sunspots could be undertaken. The great astronomer Galileo was among the first to make telescopic observations of sunspots.

Sunspots are regions of extremely strong magnetic fields (磁场) found on the sun's surface. A sunspot has a dark central core known as the umbra. The umbra is surrounded by a dark ring called the penumbra, where the magnetic field, spreads outward. Sunspots appear dark because they are giving off less radiation. They are cooler than the rest of the sun's surface.

Sunspots are frequently observed in pairs or in paired groups. The members of a spot pair are identified as the leading spot and the following spot. They are identified by their position in the pair in terms of the direction in which the sun rotates (旋转).

The number of sunspots at any one time varies. A large spot group may consist of as many as 10 groups and 300 spots across the sun. The number of spots changes in a fairly regular pattern called the sunspot cycle. The largest number occurs about every 11 years. At sunspot minimum, there are at most just a few small spots.

The average lifetime of an individual spot group is roughly one solar rotation, which is about 25 days. The most persistent large spots, however, can survive for two to three months.

Careful observations and systematic studies of sunspots

A．were made by ancient astronomers.

B．started in the early 17th century.

C．were made by Galileo only.

D．could be made without a telescope.

It's not surprising that sunspots (太阳黑子) were observed by ancient astronomers (天文学家). The largest sunspots on the sun can be seen without a telescope. It was not until the invention of the telescope (望远镜) in the early 17th century, however, that systematic studies of sunspots could be undertaken. The great astronomer Galileo was among the first to make telescopic observations of sunspots.

Sunspots are regions of extremely strong magnetic fields (磁场) found on the sun's surface. A sunspot has a dark Central core known as the umbra. The umbra is surrounded by a dark ring called the penumbra, where the magnetic field spreads outward. SunSpots appear dark because they are giving off less radiation. They are cooler than the rest of the sun's surface.

Sunspots are frequently observed in pairs or in paired groups. The members of a spot pair are identified as the leading spot and the following spot. They are identified by their position in the pair in terms of the direction in which the sun rotates (旋转).

The number of sunspots at any one time varies. A large spot group may consist of as many as 10 groups and 300 spots across the sun. The number of spots changes in a fairly regular pattern called the sunspot cycle. The largest number occurs about every 11 years. At sunspot minimum, there are at most just a few small spots.

The average lifetime of an individual spot group is roughly one solar rotation, which is about 25 days. The most persistent large spots,' however, can survive for two to three months.

Careful observations and systematic studies of sunspots

A．were made by ancient astronomers.

B．started in the early 17th century.

C．were made by Galileo only.

D．could be made without a telescope.

Sunspots

It's not surprising that sunspots（太阳黑子）were observed by ancient astronomers（天文学家）．The largest sunspots on the sun can be seen without a telescope．1t was not until the invention of the telescope（望远镜）in the early l7th century，however，that systematic studies of sunspots could be undertaken．The great astronomer Galileo was among the first to make telescopic observations of sunspots．

Sunspots are regions of extremely strong magnetic fields（磁场）found on the sun's surface．A sunspot has a dark central core known as the umbra．The umbra is surrounded by a dark ring called the penumbra．where the magnetic field spreads outward．Sunspots appear dark because they are giving off less radiation．They are cooler than the rest of the sun's surface．

Sunspots are frequently observed in pairs or in paired groups．The members of a spot pair are identified as the leading spot and the following spot．They are identified by their position In the pair In terms of the direction in which the sun rotates（旋转）．

The number of sunspots at any one time varies．A large spot group may consist of as many as 10 groups and 300 spots across the sun．The number of spots changes in a fairly regular pattern called the sunspot cycle．The largest number occurs about every 11 years．At sunspot minimum, there are at most just a few small spots．

The average lifetime of an individual spot group is roughly one solar rotation．which is about 25 days．The most persistent large spots, however, can survive for two to three months．

41 Careful observations and systematic studies of sunspots

A were made by ancient astronomers．

B started in the early 17th century．

C were made by Galileo only．

D could be made without a telescope．

Sunspots （太阳黑子）

It&39;s not surprising that sunspots were observed by ancient astronomers (天文学家) . The largest sunspots on the sun can be seen without a telescope. It was not until the invention of the telescope (望远镜) in the early 17th century, however, that systematic studies of sunspots could be undertaken. The great astronomer Galileo was among the first to make telescopic observations of sunspots.<br>

Sunspots are regions of extremely strong magnetic fields (磁场) found on the sun&39;s surface. A sunspot has a dark central core known as the umbra. The umbra is surrounded by a dark ring called the penumbra, where the magnetic field spreads outward. Sunspots appear dark because they are giving off less radiation. They are cooler than the rest of the sun&39;s surface.<br>

Sunspots are frequently observed in pairs or in paired groups. The members of a spot pair are identified as the leading spot and the following spot. They are identified by their position in the pair in terms of the direction in which the sun rotates (旋转) .<br>

The number of sunspots at any one time varies. A large spot group may consist of as many as 10 groups and 300 spots across the sun. The number of spots changes in a fairly regular pattern called the sunspot cycle. The largest number occurs about every 11 years. At sunspot minimum, there are at most just a few small spots.<br>

The average lifetime of an individual spot group is roughly one solar rotation, which is about25 days. The most persistent large spots, however, can survive for two to three months.

Careful observations and systematic studies of sunspots __________. 查看材料

A.were made by ancient astronomers

B.started in the early 17th century

C.were made by Galileo only

D.could be made without a telescope

  短暂的雷雨过后，太阳从云后面出来了。

PURCHASE CONTRACT

P/C NO：040426

DATE：15 DEC.2006

THE SELLER：Guangzhou Sun Co.，Ltd. THE BUYER：DDD Co.，Ltd.

ADDRESS：No.118 Xueyuan Street， ADDRESS：No.5 Raul Street

Guangzhou，China Hamburg，German

We hereby confirm having sold tO you the following goods on terms and conditions as stated bellows：

DESCRIPTION OF GOODS：

LADIES JACKET，woven，fur at collar，with bronze-coloured buttons，like original sample but without flaps at chest．

Shell：twill 100%cotton twill 20×16/128×60，reactive dyed，stoned washed

Lining：100%polyester 230T

Padding：100% polyester，body 140g，sleeve 120g

UNIT PRICE：USD7.10 per piece FOB GUANGZHOU

QUANTITY：14400pcs

AMOUNT：USD102240.00

More or less 1%of the quantity and the amount are allowed．

TERMS OF PAYMENT：L/C 60 days after B/L date

DATE AND METHOD OF SHIPMENT：20 June，2007 30 June，2007 by sea；otherwise 1 July，2007 15

July，2007 on seller'S account by air．

PORT OF LOADING：Guangzhou

PORT OF DESTINATION：Hamburg

PARTIAL SHIPMENT：Prohibited

SlZE/COLOR ASSORTMENT：

PURCHASE CONDYTIONS：

Attn.AZO and Nickel．

The import and sale of products with AZO-colours and nickel accessories into Germany is strictly forbidden．The supplier warrants that the manufacture of the delivered goods has not invoh,ed work by children in an exploiting，health-endangering or slavelike manner，forced labour or exploitative prison WOrk．

The material composition of each article has to be advised；for garments on the sew-in label in following languages：German，English，Spanish and French；for nontextiles on the packing according tO the special instructions which will be specified for each individual order．

If the labeling or pricing of the goods is not correct．we will debit the supplier 3% of purchase price．

Place of performance and court of jurisdiction：Dortmund/Germany．

SHIPPING MARKS：

040426

DDD

BREMEN

C.NO.：1-UP

SIDEMARKS：

LIEF-NR：70019

AUFTR.NR：040426

EKB：DOBI

WGR.：938

ST/KRTN 1/：8

SPKA2699

SPKD2499

SIGNATURE： SIGNATURE：

(SELLER) (BUYER)

订购合同审查操作

阅读理解本订购合同内容，把下列条款翻译成中文并回答相关问题。

DESCRIPTION OF GOODS：

LADIES JACKET，woven，fur at collar，with bronze-coloured buttons，like original sample but without flaps at chest．

(1) 翻译：

(2) 什么是woven面料?其基本组织有几种?