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Exam Code:
F5CAB4
Exam Name:
BIG-IP Administration Control Plane Administration
Questions:
94 Q&A
Product Type:

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NEW QUESTION: 1
A Huawei OceanStor 9000 is externally shared using NFS and CIFS at the moment.
You want to set some parameters to improve the performance of the NFS mounted under the Linux operating
system. Which of the following description is correct?
A. Async, allowing asynchronous data write, synchronous write requirements. NFS server must brush each
data into the hard disk before it can return success delay higher.
B. Noatime, if you do not need to record the file access time, you can increase this parameter to avoid
frequent access, modify the access time to open pin.
C. Nolock, if there is a shared file between NFS clients, you can use this parameter. Reduce service-side
file lock overhead.
D. Rsize / wsize, read and write the maximum size of each block, it is recommended to adjust to the
maximum. General Linux operating system environment, the maximum value of 1M.
Answer: A,B,D

NEW QUESTION: 2
Your company has a main office and a branch office.
The main office contains a file server named Server1. Server1 has the BranchCache for Network Files role service installed. The branch office contains a server named Server2. Server2 is configured as a BranchCache hosted cache server.
You need to preload the data from the file shares on Server1 to the cache on Server2.
What should you run first?
A. Set-BCCache
B. Add- BCDataCacheExtension
C. Publish-BCFileContent
D. Export-BCCachePackage
Answer: C
Explanation:
Explanation/Reference:
See step 2 below.
To prehash content and preload the content on hosted cache servers
Log on to the file or Web server that contains the data that you wish to preload, and identify the folders

and files that you wish to load on one or more remote hosted cache servers.
Run Windows PowerShell as an Administrator. For each folder and file, run either the Publish-

BCFileContent command or the Publish-BCWebContent command, depending on the type of content server, to trigger hash generation and to add data to a data package.
After all the data has been added to the data package, export it by using the Export- BCCachePackage

command to produce a data package file.
Move the data package file to the remote hosted cache servers by using your choice of file transfer

technology. FTP, SMB, HTTP, DVD and portable hard disks are all viable transports.
Import the data package file on the remote hosted cache servers by using the Import-

BCCachePackage command.
Reference: Prehashing and Preloading Content on Hosted Cache Servers (Optional)

NEW QUESTION: 3
An engineer is setting up a routing instance to route the traffic across the back-up tunnel on a deployed Cisco MPLS TE next-hop protection. Which option describes the result?
A. BGP routes that points to the link
B. an OSPF or IS-IS instance that explicitly advertises the back-up tunnel
C. a static route that points to the link
D. rerouted traffic by the back-up tunnel in the event of link failure
Answer: D
Explanation:
Explanation/Reference:
Explanation:

NEW QUESTION: 4
The discoveries of the white dwarf, the neutron star, and the black hole, coming well after the discovery of the red giant are among eh most exciting developments in decades because they may be well present physicists with their greatest challenge since the failure of classical mechanics. In the life cycle of the star, after all of the hydrogen and helium fuel has been burned, the delicate balance between the outer nuclear radiations. Pressure and the stable gravitational force becomes disturbed and slow contraction begins. As compression increases, a very dense plasma forms. If the initial star had mass of less than 1.4 solar masses (1.4 times the mass of our sun), the process ceases at the density of 1,000 tons per cubic inch, and the star becomes the white dwarf. However, if the star was originally more massive, the white dwarf plasma can't resist the gravitations pressures, and in rapid collapse, all nuclei of the star are converted to a gas of free neutrons. Gravitational attraction compresses this neutron gas rapidly until a density of 10 tons per cubic inch is reached; at this point the strong nuclear force resists further contraction. If the mass of the star was between 1.4 and a few solar masses, the process stops here, and we have a neutron star. But if the original star was more massive than a few solar masses, even the strong nuclear forces cannot resist the gravitational brunch. The neutrons are forced into one another to form heavier hadrons and these in turn coalesce to form heavier entities, of which we as yet know nothing. At this point, a complete collapse of the stellar mass occurs; existing theories predict a collapse to infinite density and infinitely small dimensions Well before this, however, the surface gravitational force would become so strong that no signal could ever leave the star - any photon emitted would fall back under gravitational attraction - and the star would become black hole in space. This gravitational collapse poses a fundamental challenge to physics. When the most widely accepted theories predict such improbable things as infinite density and infinitely small dimensions, it simply means that we are missing some vital insight. This last happened in physics in the 1930's, when we faced the fundamental paradox concerning atomic structure. At that time, it was recognized that electrons moved in table orbits about nuclei in atoms. However, it was also recognized that if charge is accelerated, as it must be to remain in orbit, it radiates energy; so, theoretically, the electron would be expected eventually to spiral into the nucleus and destroy the atom.
Studies centered around this paradox led to the development of quantum mechanics. It may well be that an equivalent t advance awaits us in investigating the theoretical problems presented by the phenomenon of gravitational collapse.
The author introduces the discussion of the paradox concerning atomic structures in order to
A. illustrate the contention that improbable things do happen in astrophysics
B. Show why it was necessary to develop quantum mechanics
C. Argue that atoms can collapse if their electrons do not remain in orbit.
D. Compare the structure of an atom with the structure of star
E. Demonstrate by analogy that a vital insight in astrophysics is missing
Answer: E
Explanation:
Explanation/Reference:
Explanation:

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