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expensive resources can be unlocked or returned to a shared pool Specifically, since the ejbPassivate() method is called upon container-initiated passivation, a developer can do hings like release locks or connections it currently has Then, when the bean instance is reactivated, these resources can be regained by properly coding the ejbActivate() method In general, understanding the contract between container and bean through a state transition diagram helps developers understand what their responsibilities are and gives them the opportunity to manage or optimize an application-specific resource unknown to the container Now that we've seen the state transition diagram, we'll look at how to code the interfaces and implementation classes for our EJB Coding the Remote Interface We'll start with the BenefitEnroller remote interface This code contains declarations for methods that are exposed to remote clients One example of a remote interface for our bean is shown in Listing 8-1 Listing 8-1 The benefitEnroller Session Bean Remote Interface.



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Using an interface to represent available functionality in a remote object is a common technique in distributed object technologies For example, in CORBA appli-cations the Interface Definition Language (IDL) describes platform-independent application objects IDL code is then used as the basis for generating client and server stubs in the desired language A remote EJB interface serves the same purpose as an IDL file for clients It simply represents remote functionality without forcing the client to know where that functionality might be located and how it's accessed Instead, it just indicates that it's available, which simplifies the job of accessing and using it, especially from the client's point of view Behind the scenes, J2EE services manage the availability and scalability of an object and its methods Conceivably, J2EE can enable highly trafficked functionality to be scalably deployed by creating EJB instances as necessary In practice, the exact details vary per J2EE implementation Coding the Home Interface As we discussed earlier, the home interface of an EJB provides factory-like methods for a session bean Thus, it merely includes create() methods that, as we will see, correspond to ejbCreate()methods in the bean class For the enefits enrollment home interface, we simply need the code shown in Listing 8-2 Listing 8-2 The BenefitEnroller Session Bean Home Interface.

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12 Stars With Magnetic Fields II Numerical simulation and rst observational results A&A, 225, 467 478 [262] Finn, GD, Kemp, JC (1974) The linear polarization of 53 Camelopardis MNRAS, 167, 375 391 [257] Gjellestad, G, Babcock, HW (1953) The magnetically variable star HD 153882 ApJ, 117, 12 20 [254] Huovelin, J, Tuominen, I, Shcherbakov, ZA (1989) The magnetic elds of late-type stars: Measurements from Line Pro les 104th IAU Colloquium on Solar and Stellar Flares, August 15 19, 1988, Stanford, CA Printed in Sol Phys, 121, 419 429 [253] Kemp, JC, Wolstencroft, RD (1973) HD 215441 and 53 Camelopardalis: Intrinsic polarization of H and the continuum ApJ, 179, L33 L37 [255, 255] Kemp, JC, Wolstencroft, RD (1974) The intrinsic linear polarization of 53 Camelopardalis and 2 Canum Venaticorum MNRAS, 166, 1 18 [257] Kemp, JC, Wolstencroft, RD, Swedlund, JB (1972) Circular polarimetry of fteen interesting objects ApJ, 177, 177 189 [258] Landol , M, Bagnulo, S, Landi Degl Innocenti, M, Landi Degl Innocenti, E, Leroy, JL (1997) Constraints on the magnetic con guration of Ap stars from simple features of observed quantities A&A, 322, 197 201 [261] Landol , M, Landi Degl Innocenti, E, Landi Degl Innocenti, M, Leroy, JL (1993) Linear polarimetry of Ap stars I A simple canonical model A&A, 272, 285 298 [260] Landstreet, JD (1980) The measurement of magnetic elds in stars AJ, 85, 611 620 [253] Landstreet, JD (1982) A search for magnetic elds in normal upper main sequence stars ApJ, 258, 639 650 [258] Landstreet, JD, Borra, EF (1977) Discovery of magnetic elds in three short-period Ap stars ApJ, 212, L43 L46 [257] Leone, F, Catanzaro, G, Catalano, S (2000) Spectropolarimetric measurements of the mean longitudinal magnetic eld of chemically peculiar stars A&A, 355, 315 326 [263] Leroy, JL (1962) Contributions a L tude de la Polarisation de la Lumi re Solaire Ann d Astr, 25, 127 164 [259] Leroy, JL (1989) The spectral variation of polarization due to magnetic intensi cation A&A, 215, 360 370 [259] Leroy, JL (1990) Broad-band polarization in crowded spectra A&A, 237, 237 242 [260] Leroy, JL (1995) Linear polarimetry of Ap stars V A general catalogue of measurements A&AS, 114, 79 104 [254, 259, 259, 261, 261, 261] Leroy, JL, Bagnulo, S, Landol , M, Landi Degl Innocenti, E, (1994) A long period model for the magnetic star Equulei A&A, 284, 174 178 [260] Leroy, JL, Landol , M, Landi Degl Innocenti, E (1993) Linear polarimetry of Ap stars II New observations with a reappraisal of former ones A&A, 270, 335 344 [260] Leroy, JL, Landol , M, Landi Degl Innocenti, E (1996) Linear polarimetry of Ap stars VI A modi ed dipolar model consistent with the observations A&A, 311, 513 522 [261] Leroy, JL, Landol , M, Landi Degl Innocenti, M, Landi Degl Innocenti, E, Bagnulo, S, Laporte, P (1995) Linear Polarimetry of Ap Stars IV The in uence of deviations from a pure dipolar model A&A, 301, 797 810 [260] Leroy, JL, Landstreet, JD, Bagnulo, S (1994) 49 Camelopardalis: an uncommon magnetic star A&A, 284, 491 498 [260] North, P, Brown, DN, Landstreet, JD (1992) The magnetic eld and period of the Ap Si star 108 Aquarii A&A, 258, 389 396 [258] Piirola, V, Tuominen, I (1981) The intrinsic polarization of the magnetic variable HD 71866 pp 283 288 in Les toiles de composition chimique anormale du d but de la s quence principale (Upper main sequence chemically peculiar stars) 23rd Li ge Astrophys Coll, Universit de Li ge [259] Polosukhina, NS (1964) Polarimetric observations of the magnetic variable HD 215441 Sov Astron, 7, 498 [254] Polosukhina, NS, Lebedeva, L (1966) Polarization and brightness variations of the magnetic variable HD 215441 ov Astron, 10, 407 410 [254] Preston, GW (1967) A statistical investigation of the orientation of magnetic axes in the periodic magnetic stars ApJ, 150, 547 550 [256] Preston, GW (1969a) The magnetic eld of HD 215441 ApJ, 156, 967 982 [256].

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run anywhere and generalizes it to include display devices and six-degrees-of-freedom input peripherals such as head trackers This write once, view everywhere nature of the new view model means that an application or applet written using the Java 3D view model can render images to a broad range of display devices, including standard computer displays, multiple-projection display rooms, and head-mounted displays, without modi cation of the scene graph It also means that the same application, once again without modi cation, can render stereoscopic views and can take advantage of the input from a head tracker to control the rendered view Java 3D s view model achieves this versatility by cleanly separating the virtual and the physical world This model distinguishes between how an application positions, orients, and scales a ViewPlatform object (a viewpoint) within the virtual world and how the Java 3D renderer constructs the nal view from that viewpoint s position and orientation The application controls the ViewPlatform s position and orientation; the renderer computes what view to render using this position and orientation, a description of the end-user s physical environment, and the user s position and orientation within the physical environment This chapter rst explains why Java 3D chose a different view model and some of the philosophy behind that choice It next describes how that model operates in the simple case of a standard computer screen without head tracking the most common case Finally, it presents the relevant parts of the API from a developer s perspective Appendix C, View Model Details, describes the Java 3D view model from an advanced developer and Java D implementor s perspective.

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